September 9, 2017 Boys

Total Page:16

File Type:pdf, Size:1020Kb

September 9, 2017 Boys 42nd Annual Rensselaer Cross Country Invitational Rensselaer Central HS - September 9, 2017 Boys 8th - Overall Results Fin Pts Time Name / Bib# / Grade Team / Posn in Team --- --- ----- ----------------------------- 1 1 10:21 Elwood, Luke #661 Gr 8 Willowcreek/1 2 2 10:24 Balagtas, Henry #603 Gr 8 West Lafayette/1 3 3 10:31 Hoffman, Justin #328 Gr 8 Kankakee Valley/1 4 4 10:31 Becker, Kolten #463 Gr 8 South Central/1 5 5 10:38 Cortez, Johnny #317 Gr 8 Kahler/1 6 6 10:41 Wright, Tommy #223 Gr 8 Grimmer/1 7 10:44 Watson, Charlie #248 Gr 8 Hanover Central/ 8 7 10:44 Hogan, Cotter #379 Gr 8 Klondike/1 9 8 10:45 Vollrath, Zach #327 Gr 8 Kahler/2 10 9 10:55 Mauder, Ryan #217 Gr 8 Grimmer/2 11 10:55 Dunn, Zach #422 Gr 8 Pierce/ 12 10 10:59 Blank, Jae #399 Gr 8 Lowell/1 13 11 11:01 Collard, Adam #330 Gr 8 Kankakee Valley/2 14 12 11:05 Mose, Conner #668 Gr 8 Willowcreek/2 15 13 11:06 Darak, Lucca #212 Gr 8 Grimmer/3 16 11:06 Noble, Bryce #245 Gr 8 Hanover Central/ 17 14 11:07 Huber, Vaughn #404 Gr 8 Lowell/2 18 15 11:14 Deedrick, Nathan #213 Gr 8 Grimmer/4 19 16 11:15 Vanderveen, Vince #326 Gr 8 Kahler/3 20 17 11:15 Gorman, Tyler #402 Gr 8 Lowell/3 21 18 11:17 Uribe, Chris #531 Gr 8 Tecumseh/1 22 19 11:18 Crampton, Leo #519 Gr 8 Tecumseh/2 23 20 11:19 Gilbert, James #546 Gr 8 Washington Twp./1 24 21 11:19 Tinsely, Eric #324 Gr 8 Kahler/4 25 22 11:21 Johnson, Justice #52 Gr 8 Benton Central/1 26 23 11:22 Ramos, Avery #218 Gr 8 Grimmer/5 27 24 11:23 Williams, Connor #278 Gr 8 Hebron/1 28 25 11:25 Bagwell, Gage #671 Gr 8 Willowcreek/3 29 26 11:25 Buchanan, Blake #49 Gr 8 Benton Central/2 30 27 11:26 Henson, Daniel #274 Gr 8 Hebron/2 31 28 11:27 Pickerill, Calvini #78 Gr 8 Central Catholic/1 32 29 11:27 Toms, Edward #614 Gr 8 West Lafayette/2 33 30 11:28 Brinkley, Andrew #543 Gr 8 Washington Twp./2 34 31 11:29 Brickner, Michael #542 Gr 8 Washington Twp./3 35 32 11:31 Bakker, Jackson #397 Gr 8 Lowell/4 36 11:31 Sanchez, Daniel #423 Gr 8 Pierce/ 37 33 11:32 Powell, Nick #659 Gr 8 Willowcreek/4 38 34 11:32 Wealing, Harrison #53 Gr 8 Benton Central/3 39 35 11:34 Fredette, Andrew #605 Gr 8 West Lafayette/3 40 36 11:35 Scott, Ranger #554 Gr 8 Washington Twp./4 41 37 11:37 Adamczyk, Matthew #271 Gr 8 Hebron/3 42 38 11:38 Donahue, Jerry #520 Gr 8 Tecumseh/3 43 39 11:40 Ojeda, Luis #526 Gr 8 Tecumseh/4 44 40 11:41 Pastrick, Max #276 Gr 8 Hebron/4 45 41 11:41 Stout, Jesse #50 Gr 8 Benton Central/4 46 11:42 Howard, Ethan #186 Gr 8 Fegely/ 47 42 11:43 Herz, Ben #333 Gr 8 Kankakee Valley/3 48 43 11:44 Gideon, Trent #329 Gr 8 Kankakee Valley/4 49 44 11:44 Gorski, Kyle #533 Gr 8 Wanatah/1 50 45 11:45 Parker, Conner #430 Gr 8 Rensselaer/1 51 46 11:46 Kerr, Ethan #502 Gr 8 Southwestern/1 52 47 11:47 Jacobo, Jesus #521 Gr 8 Tecumseh/5 53 P 11:50 Miranda, Jamie #527 Gr 8 Tecumseh/6 54 11:50 Deutscher, Zander #597 Gr 8 West Central/ 55 49 11:51 Immig, Austin #320 Gr 8 Kahler/5 56 50 11:55 Barker, Tyler #115 Gr 8 Clark/1 57 51 11:57 Obermiller, Clark #381 Gr 8 Klondike/2 58 52 11:58 Hernandez, Isreal #427 Gr 8 Rensselaer/2 59 P 11:58 Salazar, Henry #525 Gr 8 Tecumseh/7 60 12:00 Sammons, Cy #483 Gr 8 South Newton/ 61 54 12:01 Haschel, Sam #464 Gr 8 South Central/2 62 12:03 Benner, Luke #592 Gr 8 Wea Ridge/ 63 55 12:05 Sengsanith, Evan #377 Gr 8 Klondike/3 64 56 12:05 Davis, Hayden #145 Gr 8 East Tipp/1 65 P 12:08 Wilson, Josiah #221 Gr 8 Grimmer/6 66 58 12:08 Stewart, Jared #504 Gr 8 Southwestern/2 67 59 12:09 Schirm, Aidan #7 Gr 8 Battle Ground/1 68 60 12:09 Lasater, Zach #610 Gr 8 West Lafayette/4 69 61 12:12 Mehisen, Omar #201 Gr 8 Griffith/1 70 62 12:13 Garwood, Ben #534 Gr 8 Wanatah/2 71 63 12:13 Burgett, Jacob #2 Gr 8 Battle Ground/2 72 64 12:14 Hall, Brendan #382 Gr 8 Klondike/4 73 65 12:15 Kain, Matthew #608 Gr 8 West Lafayette/5 74 12:16 Taylor, Dontae #460 Gr 8 Seeger/ 75 12:17 Fincher, Tanner #69 Gr 8 Carroll/ 76 12:17 Falkenstein, Joshua #68 Gr 8 Carroll/ 77 12:18 Welch , Jeremiah #461 Gr 8 Seeger/ 78 P 12:19 Moore, Miles #321 Gr 8 Kahler/6 79 P 12:19 Schmitt, Ben #220 Gr 8 Grimmer/7 80 12:20 Chapman, Jacob #482 Gr 8 South Newton/ 81 68 12:24 Buczkowski, Adrian #376 Gr 8 Klondike/5 82 69 12:27 Farler, Anthony #273 Gr 8 Hebron/5 83 70 12:28 Maier, Rafael #673 Gr 8 Willowcreek/5 84 71 12:32 Hopkins, Alexander #428 Gr 8 Rensselaer/3 85 72 12:32 Valencia, Juan #431 Gr 8 Rensselaer/4 86 P 12:33 Schassburger, Ethan #323 Gr 8 Kahler/7 87 74 12:35 Deckard, Nolan #51 Gr 8 Benton Central/5 88 75 12:39 Nava, Mekhi #200 Gr 8 Griffith/2 89 P 12:44 Medina, Anthony #675 Gr 8 Willowcreek/6 90 77 12:45 Brody, Chamness #426 Gr 8 Rensselaer/5 91 P 12:48 Byars, J.R. #272 Gr 8 Hebron/6 92 P 12:49 Havel, Sam #378 Gr 8 Klondike/6 93 12:49 Salyer, Caleb #595 Gr 8 West Central/ 94 80 12:50 Wolstenholme, Jack #125 Gr 8 Clark/2 95 81 12:50 Parent, Liam #5 Gr 8 Battle Ground/3 96 12:51 Novak, Jackson #322 Gr 8 Kahler/8 97 82 12:51 Sheely, Bradlee #537 Gr 8 Wanatah/3 98 12:53 Franco, Cesar #425 Gr 8 Pierce/ 99 12:54 Scheub, Trey #219 Gr 8 Grimmer/8 100 12:57 Dieringer, Dylan #214 Gr 8 Grimmer/+ 101 83 12:59 Newburn, Alex #536 Gr 8 Wanatah/4 102 13:00 Zollars, Billy #523 Gr 8 Tecumseh/8 103 P 13:00 Hoffman, Trevor #275 Gr 8 Hebron/7 104 13:01 Vanderveen, Nick #325 Gr 8 Kahler/+ 105 P 13:01 Blair, Jesse #662 Gr 8 Willowcreek/7 106 86 13:08 Camp, Brandon #117 Gr 8 Clark/3 107 13:09 Fischer, Reece #660 Gr 8 Willowcreek/8 108 13:11 Creasy, John #663 Gr 8 Willowcreek/+ 109 P 13:13 Kappock, Tommy #609 Gr 8 West Lafayette/6 110 88 13:17 Murray, Brady #121 Gr 8 Clark/4 111 89 13:18 McArdle, Keegan #535 Gr 8 Wanatah/5 112 90 13:18 Swathwood, Carter #148 Gr 8 East Tipp/2 113 13:22 Tuggle, Josh #424 Gr 8 Pierce/ 114 P 13:23 Williamson, Jared #432 Gr 8 Rensselaer/6 115 P 13:25 Gustus, Jackson #606 Gr 8 West Lafayette/7 116 93 13:30 Kreinbrook, Konnor #146 Gr 8 East Tipp/3 117 P 13:30 Tan, Shannon #380 Gr 8 Klondike/7 118 95 13:34 Watson, Bobby #466 Gr 8 South Central/3 119 13:35 Berquist, Seth #670 Gr 8 Willowcreek/+ 120 13:37 Arora, Deven #602 Gr 8 West Lafayette/8 121 13:38 Rishel-Dixon, Reese #517 Gr 7 Tecumseh/+ 122 96 13:39 Sharp, Anthony #199 Gr 8 Griffith/3 123 97 13:40 Owens, Billy #77 Gr 8 Central Catholic/2 124 13:40 Fritz, Cody #318 Gr 8 Kahler/+ 125 13:42 DeMendade, Colin #664 Gr 8 Willowcreek/+ 126 13:43 Hatke, Noah #524 Gr 8 Tecumseh/+ 127 13:44 Fassoth, Luke #669 Gr 8 Willowcreek/+ 128 13:44 DeLion, Luke #604 Gr 8 West Lafayette/+ 129 13:47 Thomas, Tyler #674 Gr 8 Willowcreek/+ 130 13:48 Williams, Ryan #409 Gr 8 North Newton/ 131 13:48 Shamo, Zed #613 Gr 8 West Lafayette/+ 132 13:49 Hebert, Raphael #184 Gr 8 Fegely/ 133 13:50 Wojcik, Jason #222 Gr 8 Grimmer/+ 134 13:52 Hufford, Bryce #665 Gr 8 Willowcreek/+ 135 98 13:54 Parks, Justyn #6 Gr 8 Battle Ground/4 136 99 13:57 Matthews, Santino #405 Gr 8 Lowell/5 137 100 13:58 Digregoria, Michael #3 Gr 8 Battle Ground/5 138 13:59 Toczek, Ryder #277 Gr 8 Hebron/8 139 101 14:02 DePew, Logan #75 Gr 8 Central Catholic/3 140 102 14:04 Batinick, Jack #116 Gr 8 Clark/5 141 P 14:06 Flory, Emory #119 Gr 8 Clark/6 142 P 14:07 Carver, Anthony #400 Gr 8 Lowell/6 143 105 14:08 Elsner, AJ #76 Gr 8 Central Catholic/4 144 P 14:08 Johnson, Rudy #407 Gr 8 Lowell/7 145 107 14:11 Thomas, Peyton #202 Gr 8 Griffith/4 146 P 14:14 Pinskey, Connor #123 Gr 8 Clark/7 147 14:18 Pacheco, Alan #528 Gr 8 Tecumseh/+ 148 14:18 Armenta, Ruben #530 Gr 8 Tecumseh/+ 149 14:21 Pinskey, Collin #122 Gr 8 Clark/8 150 14:26 Casbon, Luke #58 Gr 8 Boone Grove/ 151 14:27 Hannon, Jack #403 Gr 8 Lowell/8 152 109 14:31 Bruce, Donovan #74 Gr 8 Central Catholic/5 153 110 14:34 Sampson, Will #334 Gr 8 Kankakee Valley/5 154 14:35 Cripe, Mason #401 Gr 8 Lowell/+ 155 14:36 Reck, Josh #406 Gr 8 Lowell/+ 156 111 14:41 Ryan, Nolan #470 Gr 8 South Central/4 157 112 14:44 Hooper, Giobbi #549 Gr 8 Washington Twp./5 158 14:45 Flagg, Aidan #667 Gr 8 Willowcreek/+ 159 14:45 Bolz, Mark #316 Gr 8 Kahler/+ 160 14:51 Bevan, Aidan #187 Gr 8 Gavit/ 161 P 14:52 Lukes, Kyle #550 Gr 8 Washington Twp./6 162 114 14:56 Seng, Daniel #147 Gr 8 East Tipp/4 163 P 14:57 Voll , Casey #8 Gr 8 Battle Ground/6 164 116 14:58 Gwin, Jacob #149 Gr 8 East Tipp/5 165 117 15:00 Hall, David #501 Gr 8 Southwestern/3 166 15:11 Knight, Tyler #62 Gr 8 Boone Grove/ 167 15:17 Henderson, Isaiah #185 Gr 8 Fegely/ 168 15:20 Huffman, Kevin #319 Gr 8 Kahler/+ 169 P 15:24 Borders, Sage #1 Gr 8 Battle Ground/7 170 15:25 Castillo, Josh #666 Gr 8 Willowcreek/+ 171 15:32 Smart, Andrew #475 Gr 8 South Newton/ 172 15:35 Serbenta, Hunter #124 Gr 8 Clark/+ 173 119 15:37 Henry, Brock #499 Gr 8 Southwestern/4 174 15:40 Gabbert, Ian #215 Gr 8 Grimmer/+ 175 P 15:40 Cahillane, Kevin #545 Gr 8 Washington Twp./7 176 15:42 Romero, Eduardo #522 Gr 8 Tecumseh/+ 177 121 15:43 Villarreal, Carlos #500 Gr 8 Southwestern/5 178 15:43 Villasi, Orion #383 Gr 8 Klondike/8 179 15:55 Bell, Quincy #314 Gr 8 Kahler/+ 180 122 16:02 Li , Christopher #203 Gr 8 Griffith/5 181 P 16:11 Sylvester, Grant #138 Gr 7 East Tipp/6 182 P 16:28 Williamson, Josh #332 Gr 8 Kankakee Valley/6 183 P 16:42 DeJesus, Arturo #331 Gr 8 Kankakee Valley/7 184 16:57 Benedict, Caden #593 Gr 8 Wea Ridge/ 185 126 17:03 DeYoung, Hunter #469 Gr 8 South Central/5 186 17:21 Burch, Isaiah #858 Gr 8 Fegely/ 187 17:31 Crater, Jordan #591 Gr 8 Wea Ridge/ 188 17:36 Benton, Carter #398 Gr 8 Lowell/+ 189 17:41 Sawaska, Ryan #247 Gr 8 Hanover Central/ 190 18:06 Olivetti, Charlie #4 Gr 8 Battle Ground/8 191 P 19:48 Drevalas, Evan #503 Gr 8 Southwestern/6 192 21:15 Mantis, Alex #216 Gr 8 Grimmer/+ 42nd Annual Rensselaer Cross Country Invitational Rensselaer Central HS - September 9, 2017 Boys 8th -
Recommended publications
  • The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
    THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile.
    [Show full text]
  • MAFIC ANOMOLIES in the LUNAR HIGHLANDS. T. A. Giguere1,2, B
    Lunar and Planetary Science XXXI 1760.pdf MAFIC ANOMOLIES IN THE LUNAR HIGHLANDS. T. A. Giguere1,2, B. Ray Hawke1, G. A. Smith, G. Jeffrey Taylor1, D. T. Blewett1, P. G. Lucey1, and P. D. Spudis3, 1Hawai’i Inst. of Geophys. and Planetology, University of Hawai`i, 2525 Correa Rd., Honolulu, HI 96822, 2Intergraph Corporation, 2828 Pa’a St. Ste. 2150, Honolulu, HI 96819, 3Lunar and Planetary Institute, Houston, TX 77058. Introduction Results and Discussion Ancient mare basalts deposits that have been hidden Southern Central Highlands. Most of the southern or obscured by superposed higher albedo material are portion of the lunar central highlands exhibit FeO referred to as cryptomaria [1, 2, 3]. They represent a values that range between 5 and 9 wt. % and TiO2 record of the earliest mare volcanism. Earlier remote values less than 1 wt. %. However, a small area with sensing and geologic studies have provided evidence anomalously high FeO values has been identified near for the distribution of ancient mare volcanism. the 114 km Maurolycus crater at the crater Buch B. Schultz and Spudis [4] studied the distribution of dark-haloed impact craters in the lunar highlands. Maurolycus is located at 14.0° E, 41.8° S and Buch B They suggested that basaltic volcanism predated the is located at 17.0° E, 39.9° S. last major basin-forming impacts and that early mare volcanism may have been widespread. Hawke and Bell [5, 6] used near-IR spectra to demonstrate that many dark-haloed impact craters excavated ancient mare units buried by basin and crater ejecta.
    [Show full text]
  • South Pole-Aitken Basin
    Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole.
    [Show full text]
  • Science Concept 3: Key Planetary
    Science Concept 6: The Moon is an Accessible Laboratory for Studying the Impact Process on Planetary Scales Science Concept 6: The Moon is an accessible laboratory for studying the impact process on planetary scales Science Goals: a. Characterize the existence and extent of melt sheet differentiation. b. Determine the structure of multi-ring impact basins. c. Quantify the effects of planetary characteristics (composition, density, impact velocities) on crater formation and morphology. d. Measure the extent of lateral and vertical mixing of local and ejecta material. INTRODUCTION Impact cratering is a fundamental geological process which is ubiquitous throughout the Solar System. Impacts have been linked with the formation of bodies (e.g. the Moon; Hartmann and Davis, 1975), terrestrial mass extinctions (e.g. the Cretaceous-Tertiary boundary extinction; Alvarez et al., 1980), and even proposed as a transfer mechanism for life between planetary bodies (Chyba et al., 1994). However, the importance of impacts and impact cratering has only been realized within the last 50 or so years. Here we briefly introduce the topic of impact cratering. The main crater types and their features are outlined as well as their formation mechanisms. Scaling laws, which attempt to link impacts at a variety of scales, are also introduced. Finally, we note the lack of extraterrestrial crater samples and how Science Concept 6 addresses this. Crater Types There are three distinct crater types: simple craters, complex craters, and multi-ring basins (Fig. 6.1). The type of crater produced in an impact is dependent upon the size, density, and speed of the impactor, as well as the strength and gravitational field of the target.
    [Show full text]
  • Interim Report on the Thermodynamics of Chemical Species Important in Aerospace Technology
    AFOSR SCIENTIFIC REPORT D-& AFOSR— TR— 71 — 2584 DIIMARS NATBONAL BUREAU OF STANDARDS REPORT 10 481 INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY (The previous reports in this series have the NBS Report Nos. 6297, 6484, 6645, 6928, 7093, 7192, 7437, 7587, 7796, 8033, 8186, 8504, 8628, 8919, 9028, 9389, 9500, 9601, 9803, 9905, 10004, 10074, and 10326.) U.S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS U. S. Air Force, Office of Scientific Research Agreement No. AFOSR — ISSA— 70— 0002, Project No. 9750-01. INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY 1 July 1971 Approved for Public Release; Distribution Unlimited Qualified requestors may obtain additional copies from the Defense Decumentation Center; all others should apply to the Clearinghouse for Federal Scientific and Technical Information. NATIONAL BUREAU OF STANDARDS REPORT NBS PROJECT NBS REPORT 2320423 1 July 1971 10 481 3160401 3160404 3160405 3160426 INTERIM REPORT ON THE THERMODYNAMICS OF CHEMICAL SPECIES IMPORTANT IN AEROSPACE TECHNOLOGY (The previous reports in this series have the NBS Report Nos. 6297, 6484, 6645, 6928, 7093, 7192, 7437, 7587, 7796, 8033, 8186, 8504, 8628, 8919, 9028, 9389, 9500, 9601, 9803, 9905, 10004, 10074, and 10326.) Reference: U. S. Air Force, Office of Scientific Research, Agreement No. AFOSR — ISSA — 70— 0002, Project No. 9750-01. IMPORTANT NOTICE NATIONAL BUREAU OF ST iss accounting documents intended for use within the Government, ; subjected to additional evaluation Approved for public release by the and review. For this reason, th 3 listing of this Report, either in whole or in part, is not autho Director of the National Institute of le Office of the Director, National Bureau of Standards, Washingt Standards and Technology (NIST) by the Government agency for which the Report has been speciticall) copies for its own use.
    [Show full text]
  • History of the 745Th Tank Battalion, August 1942 to June 1945 Harold D
    Bangor Public Library Bangor Community: Digital Commons@bpl World War Regimental Histories World War Collections 1945 History of the 745th Tank Battalion, August 1942 to June 1945 Harold D. Howenstine Follow this and additional works at: http://digicom.bpl.lib.me.us/ww_reg_his Recommended Citation Howenstine, Harold D., "History of the 745th Tank Battalion, August 1942 to June 1945" (1945). World War Regimental Histories. 21. http://digicom.bpl.lib.me.us/ww_reg_his/21 This Book is brought to you for free and open access by the World War Collections at Bangor Community: Digital Commons@bpl. It has been accepted for inclusion in World War Regimental Histories by an authorized administrator of Bangor Community: Digital Commons@bpl. For more information, please contact [email protected]. L HISTORY- of the 745th TANK BATTALION ........ ... "·- ... " ..... .., to ~ ..... • ~ J ~ .... ,. - .. ~ ~ ~ .. .., -.. .. ... .. ., .. - .., .., J .............. " .. ... J J ... ... PRINTED IN NORNBERG, GERMANY • ...... .. ....... • -~ r,. ......... .,., . : . ..... ·.; . ..·· .... ' .. ; . .... ee-"U . "' "'"" . ,. " ; .... ... ....... ,, ~ .. .,• ! ~ .....·= w :.. To Sgt. Charles N. Donoghue, the first member of the 7 450. Tank Battalion to lose his life in combat, this history is humbly dedicated. - ' l'able of Contents Dedication Foreword Tribute by Lt. Col. Nichols Coat-of-Arms Col. Evans 1 Lt. Col. Nichols . 2 Major Heard and Major Patterson . 3 Battalion Headquarters . 5 Headquarters Company 7 Service Company 10 Company "A" 13 Company "B" 17 Company "C" 21 Company "D" 25 ~ Awards 29 Tribute to Battalion's Dead . 32 Battlefield Commissions 35 Chapters: I. Activation and Training II. The Normandy Beachhead III. The St. Lo Breakthrough IV. The Falaise Pocket V . Northern France VI. The Battle of Mons VII. The Siegfried Line VIII.
    [Show full text]
  • The Development of the Quantum-Mechanical Electron Theory of Metals: 1928---1933
    The development of the quantum-mechanical electron theory of metals: 1S28—1933 Lillian Hoddeson and Gordon Bayrn Department of Physics, University of Illinois at Urbana-Champaign, Urbana, illinois 6180f Michael Eckert Deutsches Museum, Postfach 260102, 0-8000 Munich 26, Federal Republic of Germany We trace the fundamental developments and events, in their intellectual as well as institutional settings, of the emergence of the quantum-mechanical electron theory of metals from 1928 to 1933. This paper contin- ues an earlier study of the first phase of the development —from 1926 to 1928—devoted to finding the gen- eral quantum-mechanical framework. Solid state, by providing a large and ready number of concrete prob- lems, functioned during the period treated here as a target of application for the recently developed quan- tum mechanics; a rush of interrelated successes by numerous theoretical physicists, including Bethe, Bloch, Heisenberg, Peierls, Landau, Slater, and Wilson, established in these years the network of concepts that structure the modern quantum theory of solids. We focus on three examples: band theory, magnetism, and superconductivity, the former two immediate successes of the quantum theory, the latter a persistent failure in this period. The history revolves in large part around the theoretical physics institutes of the Universi- ties of Munich, under Sommerfeld, Leipzig under Heisenberg, and the Eidgenossische Technische Hochschule (ETH) in Zurich under Pauli. The year 1933 marked both a climax and a transition; as the lay- ing of foundations reached a temporary conclusion, attention began to shift from general formulations to computation of the properties of particular solids. CONTENTS mechanics of electrons in a crystal lattice (Bloch, 1928); these were followed by the further development in Introduction 287 1928—1933 of the quantum-mechanical basis of the I.
    [Show full text]
  • Science Concept 3: Key Planetary Processes Are Manifested in the Diversity of Lunar Crustal Rocks
    Science Concept 3: Key Planetary Processes are Manifested in the Diversity of Lunar Crustal Rocks Science Concept 3: Key planetary processes are manifested in the diversity of crustal rocks Science Goals: a. Determine the extent and composition of the primary feldspathic crust, KREEP layer, and other products of differentiation. b. Inventory the variety, age, distribution, and origin of lunar rock types. c. Determine the composition of the lower crust and bulk Moon. d. Quantify the local and regional complexity of the current lunar crust. e. Determine the vertical extent and structure of the megaregolith. INTRODUCTION Formation and Evolution of the Moon The Moon is a unique environment, preserving crucial information about the early history and later evolution of the solar system. The lack of major surficial tectonic processes within the past few billion years or so, as well as the lack of significant quantities of surface water, have allowed for excellent preservation of the lithologies and geomorphological features that formed during the major planetary formation events. Fundamental discoveries during the Apollo program showed that the Moon is made up of a variety of volcanic and impact rock types that exhibit a particular range of chemical and mineralogical compositions. The key planetary processes conveyed by this diversity include planetary differentiation, volcanism, and impact cratering. Analysis of Apollo, Luna, and lunar meteoritic samples, as well as orbital data from a series of lunar exploration missions, generated geophysical models that strove to tell the story of the Moon. However, such models are restricted in the sense that they are based on information gathered from the samples that have so far been acquired.
    [Show full text]
  • Basic Optical Properties of Materials Summaries of Papers NATIONAL BUREAU of STANDARDS
    A111D3 QSb3SS NATL INST OF STANDARDS & TECH RI.C. A1 11 03056385 _ Conference o/Basic optical prope 100 U57 N0.574, 1980 C.1 NBS-PUB-C 19 NBS SPECIAL PUBLICATION 574 * V„U Of U.S. DEPARTMENT OF COMMERCE / National Bureau of Standards Basic Optical Properties of Materials Summaries of Papers NATIONAL BUREAU OF STANDARDS The National Bureau of Standards' was established by an act of Congress on March 3, 1901. The Bureau's overall goal is to strengthen and advance the Nation's science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research and provides: (1) a basis for the Nation's physical measurement system, (2) scientific and technological services for industry and government, (3) a technical basis for equity in trade, and (4) technical services to promote public safety. The Bureau's technical work is per- formed by the National Measurement Laboratory, the National Engineering Laboratory, and the Institute for Computer Sciences and Technology. THE NATIONAL MEASUREMENT LABORATORY provides the national system ot physical and chemical and materials measurement; coordinates the system with measurement systems of other nations and furnishes essential services leading to accurate and uniform physical and chemical measurement throughout the Nation's scientific community, industry, and commerce; conducts materials research leading to improved methods of measurement, standards, and data on the properties of materials needed by industry, commerce, educational institutions, and Government; provides advisory and research services to other Government agencies; develops, produces, and distributes Standard Reference Materials; and provides calibration services. The Laboratory consists of the following centers: Absolute Physical Quantities 2 — Radiation Research — Thermodynamics and Molecular Science — Analytical Chemistry — Materials Science.
    [Show full text]
  • Innovation & Intersection
    FORESTSAMERICAN FALL 2017 INNOVATION & INTERSECTION PEOPLE, PLACES AND PROFESSIONS AT THE CENTER OF VIBRANT CITIES One Tree Planted for Every Tree Sold When you shop fresh ingredients for your holiday feast, pick a tree, too. Because with every in-store purchase of a full-size Christmas tree, Whole Foods Market® makes a donation to American Forests to plant new evergreens in state and national forests. So go ahead: deck the halls, set the table, and help us fi ll the forest. wholefoodsmarket.com VOL 123 NO 3 CONTENTS FALL 2017 Departments 16 24 2 Offshoots A word from our Vice President of Conservation Programs 4 Treelines From Washington, D.C. to our Facebook community, here’s what we’ve been up to and talking about on the Hill and online. Plus, FOREST FRONTIERS: LAURENCE Wiseman, Chair of the National Urban and Community Forestry Advisory Council, shares what led him to work in urban forestry and the challenges facing the field. NEW ONLINE: Discover why our Facebook community believes wildlife conservation is so 32 40 important. WASHINGTON OUTLOOK: A look at the impact of proposed budget cuts on important forestry and conservation programs. 40 Vibrant Cities Lab By Ian Leahy Introducing a new state-of- the-art platform designed to bring together urban forestry professionals and recourses in one place. 46 Earthkeepers It Starts with a Fever Read the inspiring story of Melissa Jenkins, a woman with a mission Features and a passion for protecting the whitebark pine. 48 Last Look 16 24 32 A look at a very rare West Coast Woodpeckers: One Tree, Timberline forest ecosystem: photography from Chuck Graham The Engineers Many Futures By Ian Vorster of Ecosystems By Doyle Irvin Follow a hiker as he By Jared Lloyd Learn about the fight to traverses the infamous John Discover how one species save the whitebark pine, a Muir Trail, a recreation can have a profound impact keystone species destination transforming in on the entire longleaf pine on the brink of extinction, the tumult of climate change.
    [Show full text]
  • Historical Natural Kinds and Mineralogy: Systematizing Contingency in the Context PERSPECTIVE of Necessity Carol E
    PERSPECTIVE Historical natural kinds and mineralogy: Systematizing contingency in the context PERSPECTIVE of necessity Carol E. Clelanda, Robert M. Hazenb,1, and Shaunna M. Morrisonb Edited by Bruce Watson, Rensselaer Polytechnic Institute, Troy, NY, and approved November 2, 2020 (received for review July 20, 2020) The advancement of science depends upon developing classification protocols that systematize natural objects and phenomena into “natural kinds”—categorizations that are conjectured to represent genuine divisions in nature by virtue of playing central roles in the articulation of successful scientific theories. In the physical sciences, theoretically powerful classification systems, such as the periodic table, are typically time independent. Similarly, the standard classification of mineral species by the International Mineralogical Association’s Commission on New Minerals, Nomenclature, and Classification relies on idealized chemical composition and crystal structure, which are time-independent attributes selected on the basis of theo- retical considerations from chemical theory and solid-state physics. However, when considering mineral kinds in the historical context of planetary evolution, a different, time-dependent classification scheme is warranted. We propose an “evolutionary” system of mineral classification based on recognition of the role played by minerals in the origin and development of planetary systems. Lacking a comprehensive theory of chemical evolution capable of explaining the time-dependent pattern of chemical
    [Show full text]
  • Image Map of the Moon
    U.S. Department of the Interior Prepared for the Scientific Investigations Map 3316 U.S. Geological Survey National Aeronautics and Space Administration Sheet 1 of 2 180° 0° 5555°° –55° Rowland 150°E MAP DESCRIPTION used for printing. However, some selected well-known features less that 85 km in diameter or 30°E 210°E length were included. For a complete list of the IAU-approved nomenclature for the Moon, see the This image mosaic is based on data from the Lunar Reconnaissance Orbiter Wide Angle 330°E 6060°° Gazetteer of Planetary Nomenclature at http://planetarynames.wr.usgs.gov. For lunar mission C l a v i u s –60°–60˚ Camera (WAC; Robinson and others, 2010), an instrument on the National Aeronautics and names, only successful landers are shown, not impactors or expended orbiters. Space Administration (NASA) Lunar Reconnaissance Orbiter (LRO) spacecraft (Tooley and others, 2010). The WAC is a seven band (321 nanometers [nm], 360 nm, 415 nm, 566 nm, 604 nm, 643 nm, and 689 nm) push frame imager with a 90° field of view in monochrome mode, and ACKNOWLEDGMENTS B i r k h o f f Emden 60° field of view in color mode. From the nominal 50-kilometer (km) polar orbit, the WAC This map was made possible with thanks to NASA, the LRO mission, and the Lunar Recon- Scheiner Avogadro acquires images with a 57-km swath-width and a typical length of 105 km. At nadir, the pixel naissance Orbiter Camera team. The map was funded by NASA's Planetary Geology and Geophys- scale for the visible filters (415–689 nm) is 75 meters (Speyerer and others, 2011).
    [Show full text]