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Spring 2008 (PDF)
SKYWARNEWS National Weather Service State College, PA Spring/Summer 2008 “Working Together To Save Lives” The Cooperative Observers meteorological data in near real-time, to support forecast, warning and other public – Creators of Our service programs of the National Weather Country’s Weather History Service. By Victor Cruz, Observation Program Volunteers in the Cooperative Program are Leader trained by National Weather Service personnel and receive the equipment to And so, my fellow Americans: ask not perform their duties. In Central what your country can do for you—ask Pennsylvania, the oldest and longest what you can do for your country. The continuous Cooperative Program is located aforementioned sentence was uttered by in Lancaster County. The City of Lancaster President John F. Kennedy during his Filter Plant has been a cooperative weather Inaugural Address on January 20, 1961. site since May 01, 1887. Our newest However, long before President Kennedy Cooperative Observer is in Chandler’s had spoken those words, the Cooperative Valley, which was established on June 19, Weather Observer Program had been in 2004. Approximately 115 cooperative full swing, since its creation in 1890 under observers help to maintain the Cooperative the Organic Act. Observer Program in Central Pennsylvania. The National Weather Service (NWS) Everyday more than 12,000 weather Cooperative Observer Program (COOP) is volunteers take cooperative observations truly the Nation's weather and climate on farms, at homes in urban and suburban observing network of, by and for the areas, National Parks, seashores, and people. mountaintops. The data they collect are an invaluable measurement of atmospheric The basic equipment for most new Coop conditions where people live, work and Stations is a Standard Rain Gage, play. -
Navigating North America
deep-sky wonders by sue french Navigating North America the north america nebula is one of the most impres- NGC 6997 is the most obvious cluster within the confines sive nebulae glowing in our sky. This nebula’s remarkable of the North America Nebula. To me, it looks as though it’s resemblance to the North American continent makes it bet- been plunked down on the border between Ohio and West ter known by its common name — bestowed not by a resi- Virginia. Putting 4.8-magnitude 57 Cygni at the western dent of North America, but by German astrono- edge of a low-power eyepiece field should bring NGC 6997 Knowing mer Max Wolf. In 1890 Wolf became the first into view. My 4.1-inch scope at 17× displays a dusting of person to photograph the North America Nebula, very faint stars. At 47×, it’s a pretty cluster, rich in faint your and for many years this remained the only way to stars, spanning 10′. Through my 10-inch reflector, I count geography fully appreciate its distinctive shape. With today’s 40 stars, mostly of magnitude 11 and 12. Many are abundance of short-focal-length telescopes and arranged in two incomplete circles, one inside the other. puts you wide-field eyepieces, we can more readily enjoy Is NGC 6997 actually involved in the North America one step this large nebula visually. Nebula? It’s difficult to tell because the distances are poorly The North America Nebula, NGC 7000 or Cald- known. A journal article earlier this year puts NGC 6997 at ahead in well 20, is certainly easy to locate. -
Arxiv:2012.09981V1 [Astro-Ph.SR] 17 Dec 2020 2 O
Contrib. Astron. Obs. Skalnat´ePleso XX, 1 { 20, (2020) DOI: to be assigned later Flare stars in nearby Galactic open clusters based on TESS data Olga Maryeva1;2, Kamil Bicz3, Caiyun Xia4, Martina Baratella5, Patrik Cechvalaˇ 6 and Krisztian Vida7 1 Astronomical Institute of the Czech Academy of Sciences 251 65 Ondˇrejov,The Czech Republic(E-mail: [email protected]) 2 Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetsky pr. 13, 119234, Moscow, Russia 3 Astronomical Institute, University of Wroc law, Kopernika 11, 51-622 Wroc law, Poland 4 Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotl´aˇrsk´a2, 611 37 Brno, Czech Republic 5 Dipartimento di Fisica e Astronomia Galileo Galilei, Vicolo Osservatorio 3, 35122, Padova, Italy, (E-mail: [email protected]) 6 Department of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University in Bratislava, Mlynsk´adolina F-2, 842 48 Bratislava, Slovakia 7 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, H-1121 Budapest, Konkoly Thege Mikl´os´ut15-17, Hungary Received: September ??, 2020; Accepted: ????????? ??, 2020 Abstract. The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters. As a result, 56 flare stars were found, among them 8 hot B-A type ob- jects. Of all flares, 63 % were detected in sample of cool stars (Teff < 5000 K), and 29 % { in stars of spectral type G, while 23 % in K-type stars and ap- proximately 34% of all detected flares are in M-type stars. -
A Campus Observatory Image of the North America Nebula
The Observer A Campus Observatory Image of the North America Nebula by Fred Ringwald Fresno State’s Campus Observatory is convenient for students to use, but its sky rates 10 on the Bortle scale: “Most people don’t look up.” The faintest stars the unaided eye can see there are about 3rd magnitude. Nevertheless, its telescopes can get good images through an Hα (pronounced “H-alpha”) filter. An Hα filter passes only a narrow band of wavelengths that are centered on the Hα line, the scarlet wavelength at which hydrogen radiates the most light visible to the eye. City lights radiate mostly at other wavelengths, from mercury or sodium vapor in the lamps. Hydrogen is the most common element in nebulae, so Hα filters improve their image contrast. This image was taken through a 70-mm guidescope mounted piggyback on the Campus Observatory’s main telescope. The guidescope was made by Vixen. With a focal length of only 400 mm, the guidescope gets a wide field of view, which makes it easier for novice students to point the telescope. With the SBIG ST-9 camera used to take this image, the field of view is 1.5º on a side. It shows the southern end of NGC 7000, called “the North America Nebula” because of its shape. At upper right is “Florida,” bounded by a dust lane corresponding to the “Gulf of Mexico”; at bottom-center is “Mexico.” A bright shock front runs through the east side (on the left), which is called “the Great Wall,” incongruous since that’s in China! The North America Nebula is in the constellation Cygnus, 3º east of the 1st-magntude supergiant star Deneb. -
J Pionisrskis Lata Eieitronorriii W Toruniu
j Pionisrskis lata EiEitronorriii w Toruniu j Aktywność magnetyczna Słońca j Towarzyskie pJaneioidy Pawilon teleskopu Schmidta-Cassegraina w Piwnicach od strony południowo-zachodniej stu Mikołaja Kopernika prawie w komplecie — październik 2005 r. Szanowni i Drodzy Czytelnicy, Prenumeratorów naszego czasopisma spotyka w tym miesiącu nagroda — wszyscy otrzymują dwa zeszyty „ Uranii-Postępów Astronomii”. Jeden, to regularny zeszyt noszący datę marzec-kwiecień 2006 r., a drugi to bonus — specjalne wydanie „ Uranii”. Zawiera ono referaty wygłoszone na angielskojęzycznych sesjach w czasie Zjazdu Polskiego Towarzystwa fot. bauksza-WiiniewsltaA. Astronomicznego we wrześniu 2005 r. we Wrocławiu. Skupiają się one wokół dwóch zagadnień: gwiazd pulsujących (w tym astrosejsmologii) i fizyki Słońca. Autorzy są znakomitymi specjalistami tych dziedzin, a całość stanowi doskonały obraz problemów współczesnych astronomii w tych tematach. Komitet Organizacyjny Zjazdu znalazł pieniądze na wydanie materiałów zjazdowych i zrobienie prezentu naszym najwierniejszym Czytelnikom, za co jesteśmy mu bardzo wdzięczni. Nasz zwykły, polskojęzyczny nr 2 (722) otwiera, kreślone piórem niżej podpisanego, wspomnienie pionierskich lat astronomii w Toruniu, rodzącej się wraz z powstaniem Uniwersytetu Mikołaja Kopernika. Uniwersytet ten świętował w 2005 r. swoje 60-łecie. Uznaliśmy, że wypada też przypomnieć z tej okazji, jak to się narodził i rósł toruński ośrodek astronomiczny, który dzisiaj nosi miano Centrum Astronomii UMK. Następnie naszą uwagę kierujemy na najważniejszy obiekt nieba — Słońce. O badaniu naszej dziennej gwiazdy i procesach zachodzących w jej zewnętrznych warstwach opowiada hełiofizyk Paweł Rudawy z Wrocławia. Analizuje głównie zjawiska zachodzące między polem magnetycznym a plazmą słoneczną. Oddziaływania te leżą u podstaw zjawisk tzw. aktywności słonecznej, które są pilnie obserwowane nie tylko przez profesjonalnych astronomów, ale też i przez tysiące miłośników astronomii. -
Binocular Challenge Here
AHSP Binocular Observing Award Compiled by Phil Harrington www.philharrington.net • To qualify for the BOA pin, you must see 15 of the following 20 binocular targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 2. M57 Lyr PN 18 53.6 +33 02 9.7 86"x62" Ring Nebula 3. Collinder 399 Vul AS 19 25.4 +20 11 3.6 60' Coathanger/Brocchi’s Cluster 3.1 4. Albireo Cyg Dbl 19 30.7 +27 57 35” Color Contrasting Double 5.1 5. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 6. NGC 6992 Cyg SNR 20 56.4 +31 43 - 60'x8 Veil Nebula (east) 7. NGC 7000 Cyg BN 20 58.8 +44 20 - 120'x100' North America Nebula 8. M15 Peg GC 21 30.0 +12 10 7.5 12’ Great Pegasus Cluster 9. M39 Cyg OC 21 32.2 +48 26 4.6 32' 10. Barnard 168 Cyg DN 21 53.2 +47 12 - 100'x10' West of Cocoon Nebula 11. IC 5146 Cyg BN/OC 21 53.5 +47 16 - 12'x12' Cocoon Nebula 12. M110 And Gx 00 40.4 +41 41 10 17’x10’ 13. M32 And Gx 00 42.8 +40 52 10 8’x6’ 14. M31 And Gx 00 42.8 +41 16 4.5 178’ Andromeda Galaxy 15. NGC 457 Cas OC 01 19.1 +58 20 6.4 13’ Owl Cluster/ET Cluster 16. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
USBC Approved Bowling Balls
USBC Approved Bowling Balls (See rulebook, Chapter VII, "USBC Equipment Specifications" for any balls manufactured prior to January 1991.) ** Bowling balls manufactured only under 13 pounds. 5/17/2011 Brand Ball Name Date Approved 900 Global Awakening Jul-08 900 Global BAM Aug-07 900 Global Bank Jun-10 900 Global Bank Pearl Jan-11 900 Global Bounty Oct-08 900 Global Bounty Hunter Jun-09 900 Global Bounty Hunter Black Jan-10 900 Global Bounty Hunter Black/Purple Feb-10 900 Global Bounty Hunter Pearl Oct-09 900 Global Break Out Dec-09 900 Global Break Pearl Jan-08 900 Global Break Point Feb-09 900 Global Break Point Pearl Jun-09 900 Global Creature Aug-07 900 Global Creature Pearl Feb-08 900 Global Day Break Jun-09 900 Global DVA Open Aug-07 900 Global Earth Ball Aug-07 900 Global Favorite May-10 900 Global Head Hunter Jul-09 900 Global Hook Dark Blue/Light Blue Feb-11 900 Global Hook Purple/Orange Pearl Feb-11 900 Global Hook Red/Yellow Solid Feb-11 900 Global Integral Break Black Nov-10 900 Global Integral Break Rose/Orange Nov-10 900 Global Integral Break Rose/Silver Nov-10 900 Global Link Jul-08 900 Global Link Black/Red Feb-09 900 Global Link Purple/Blue Pearl Dec-08 900 Global Link Rose/White Feb-09 900 Global Longshot Jul-10 900 Global Lunatic Jun-09 900 Global Mach One Blackberry Pearl Sep-10 900 Global Mach One Rose/Purple Pearl Sep-10 900 Global Maniac Oct-08 900 Global Mark Roth Ball Jan-10 900 Global Missing Link Black/Red Jul-10 900 Global Missing Link Blackberry/Silver Jul-10 900 Global Missing Link Blue/White Jul-10 900 Global -
Sky & Telescope
Eclipse from the See Sirius B: The Nearest Spot the Other EDGE OF SPACE p. 66 WHITE DWARF p. 30 BLUE PLANETS p. 50 THE ESSENTIAL GUIDE TO ASTRONOMY What Put the Bang in the Big Bang p. 22 Telescope Alignment Made Easy p. 64 Explore the Nearby Milky Way p. 32 How to Draw the Moon p. 54 OCTOBER 2013 Cosmic Gold Rush Racing to fi nd exploding stars p. 16 Visit SkyandTelescope.com Download Our Free SkyWeek App FC Oct2013_J.indd 1 8/2/13 2:47 PM “I can’t say when I’ve ever enjoyed owning anything more than my Tele Vue products.” — R.C, TX Tele Vue-76 Why Are Tele Vue Products So Good? Because We Aim to Please! For over 30-years we’ve created eyepieces and telescopes focusing on a singular target; deliver a cus- tomer experience “...even better than you imagined.” Eyepieces with wider, sharper fields of view so you see more at any power, Rich-field refractors with APO performance so you can enjoy Andromeda as well as Jupiter in all their splendor. Tele Vue products complement each other to pro- vide an observing experience as exquisite in performance as it is enjoyable and effortless. And how do we score with our valued customers? Judging by superlatives like: “in- credible, truly amazing, awesome, fantastic, beautiful, work of art, exceeded expectations by a mile, best quality available, WOW, outstanding, uncom- NP101 f/5.4 APO refractor promised, perfect, gorgeous” etc., BULLSEYE! See these superlatives in with 110° Ethos-SX eye- piece shown on their original warranty card context at TeleVue.com/comments. -
Meteor Showers # 11.Pptx
20-05-31 Meteor Showers Adolf Vollmy Sources of Meteors • Comets • Asteroids • Reentering debris C/2019 Y4 Atlas Brett Hardy 1 20-05-31 Terminology • Meteoroid • Meteor • Meteorite • Fireball • Bolide • Sporadic • Meteor Shower • Meteor Storm Meteors in Our Atmosphere • Mesosphere • Atmospheric heating • Radiant • Zenithal Hourly Rate (ZHR) 2 20-05-31 Equipment Lounge chair Blanket or sleeping bag Hot beverage Bug repellant - ThermaCELL Camera & tripod Tracking Viewing Considerations • Preparation ! Locate constellation ! Take a nap and set alarm ! Practice photography • Location: dark & unobstructed • Time: midnight to dawn https://earthsky.org/astronomy- essentials/earthskys-meteor-shower- guide https://www.amsmeteors.org/meteor- showers/meteor-shower-calendar/ • Where to look: 50° up & 45-60° from radiant • Challenges: fatigue, cold, insects, Moon • Recording observations ! Sky map, pen, red light & clipboard ! Time, position & location ! Recording device & time piece • Binoculars Getty 3 20-05-31 Meteor Showers • 112 confirmed meteor showers • 695 awaiting confirmation • Naming Convention ! C/2019 Y4 (Atlas) ! (3200) Phaethon June Tau Herculids (m) Parent body: 73P/Schwassmann-Wachmann Peak: June 2 – ZHR = 3 Slow moving – 15 km/s Moon: Waning Gibbous June Bootids (m) Parent body: 7p/Pons-Winnecke Peak: June 27– ZHR = variable Slow moving – 14 km/s Moon: Waxing Crescent Perseid by Brian Colville 4 20-05-31 July Delta Aquarids Parent body: 96P/Machholz Peak: July 28 – ZHR = 20 Intermediate moving – 41 km/s Moon: Waxing Gibbous Alpha -
Meteor- Scatter
Catch a Falling Star A beginner’s guide to meteor-scatter communication— just in time for “stormy” weather! By Kirk Kleinschmidt, NT0Z Newcomers to Amateur Radio usually have a few misconceptions about VHF propagation. The worst—which is often “propagated” by more experienced hams who should know better—suggests that VHF signals travel exclusively along line-of-sight paths and peter out after about 30 miles. That’s far from true, but if your VHF operation is limited to 2-meter FM it’s somehow practical, especially if you’re using a hand-held radio and a rubber ducky antenna. Once you cross the “30-mile barrier,” however, there are many exciting and interesting ways to propagate your VHF signal hundreds or even thousands of kilometers. Articles in the ARRL Operating Manual and QST detail E- and F-layer skip, tropospheric ducting and transequatorial field-aligned irregularities, moon-bounce, auroral propagation and others. These modes aren’t always casual. That is, many require robust stations, high power and more than a little patience. Meteor- scatter work—bouncing radio signals off the ionized trails produced by meteors burning through the ionosphere—doesn’t require an extraordinary station, but some patience is usually necessary unless you know exactly when conditions may be favorable! That’s precisely the case with the November Leonids meteor showers for the next few years. (Meteor showers are named for the constellations from which they seem to appear. Meteors produced during the recurring November 17 shower seem to “pour” from the constellation Leo.) As an added bonus, on one or more of those November days the short-duration, high-intensity Leonids have the potential to produce the best meteor-scatter propagation since November 1966 (and a spectacular light show if you’re on the night side of the planet!). -
Stellar Chromospheric Activity and Age Relation from Open Clusters in the LAMOST Survey
Publications 12-12-2019 Stellar Chromospheric Activity and Age Relation from Open Clusters in the LAMOST Survey Jiajun Zhang University of Chinese Academy of Sciences, Terry Oswalt Embry-Riddle Aeronautical University, [email protected] Jingkun Zhao University of Chinese Academy of Sciences, Xiangsong Fang National Astronomical Observatories Gang Zhao Chinese Academy of Sciences, See next page for additional authors Follow this and additional works at: https://commons.erau.edu/publication Part of the Stars, Interstellar Medium and the Galaxy Commons Scholarly Commons Citation Zhang, J., Oswalt, T., Zhao, J., Fang, X., Zhao, G., Liang, X., Ye, X., & Zhong, J. (2019). Stellar Chromospheric Activity and Age Relation from Open Clusters in the LAMOST Survey. The Astrophysical Journal, 887(1). Retrieved from https://commons.erau.edu/publication/1383 This Article is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Authors Jiajun Zhang, Terry Oswalt, Jingkun Zhao, Xiangsong Fang, Gang Zhao, Xilong Liang, Xianhao Ye, and Jing Zhong This article is available at Scholarly Commons: https://commons.erau.edu/publication/1383 Draft version October 1, 2019 Typeset using LATEX default style in AASTeX62 Stellar chromospheric activity and age relation from open clusters in the LAMOST Survey Jiajun Zhang,1, 2 Jingkun Zhao,1 Terry D. Oswalt,3 Xiangsong Fang,4, 5 Gang Zhao,1, 2 Xilong Liang,1, 2 Xianhao Ye,1, 2 and Jing Zhong6 1Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China.