Parker Solar Probe SWG Telecon February 5, 2020 Project Science Report Nour Raouafi Project Status Helene Winters Payload Status SB,JK,DM,RH Solar Orbiter H. Gilbert/C. St. Cyr SOC Activities Martha Kusterer Payload SE Telecon S. Hamilton/A. Reiter Theory Group M. Velli/A. Higginson Upcoming Meetings Nour Raouafi Science Presentations: DaviD Malaspina (LASP) & Karl Battams (NRL) Agenda • DCP 5 Information • DCP Type: Data Volume • Venus Flyby • Non-routine Activities & Science Priorities o WISPR o ISOIS o FIELDS o SWEAP • Modeling – Robert Allen • Coordinated observations. Parker Solar Probe Project Science SWG Telecon February 5, 2020 ApJS Special Issue (ApJ/SI) 50+ papers submitted as of Oct. 20, 2019 Early Results from Parker Solar Probe: Ushering a New Frontier in Space Exploration • Publication Date: February 3, 2020 • 48 papers accessible online • Few more papers still under review Corresponding authors: please speed up the reviewing process – Send me your submission info and the manuscript. • Print copies: Science Teams are you interested in ordering print copies of the special issue? 2/7/20 4 Nature Papers ADS not listing all the authors • ADS lists only three authors: the first two and the last one • The issue was addressed for the FIELDS and WISPR papers • But not for the SWEAP and ISOIS papers • ADS stated that that’s the information Nature sent to them • Corrections can submitted through http://adsabs.harvard.edu/adsfeedback/submit_abstract.php. 2/7/20 5 Future Publications • Let’s us know about your results in case we need to prepare for press releases • Animations take time to design and get ready • Please do not for the mission acknowledgements Parker Solar Probe was designed, built, and is now operated by the Johns Hopkins Applied Physics Laboratory as part of NASA’s Living with a Star (LWS) program (contract NNN06AA01C). Support from the LWS management and technical team has played a critical role in the success of the Parker Solar Probe mission. 2/7/20 6 Parker One March 23-27, 2020 • 182 abstract submitted so far • Submission will remain open for late abstracts • ~150 attendees registered If you have not registered yet, please consider to do so soon • Hotels, info website Parker One Science Program • Science Organizing Committee: Marco Velli (Co-Chair), Nicholeen Viall (Co-Chair), Stuart Bale, Benjamin Chandran, Christina Cohen, Rob Decker, Aleida Higginson, Russell Howard, Colin Joyce, Justin Kasper, David Lario, David J. McComas, Nour E. Raouafi, Adam Szabo, Anna Tenerani, Angelos Vourlidas • 13 Invited talks • 40 Contributed talks • Two poster sessions, ~70 posters each 1st session: Monday-Tuesday 2nd session: Wednesday-Thursday • Data tutorials Marc Pulupa (FIELDS) Tony Case (SWEAP) Nathan Schwadron (ISOIS) Guillermo Stenborg (WISPR) Space- and Ground-based Support Encounter 4 and beyond ~50 observatories around the globe support Parker Enc. 4 • Space: Hinode, IRIS, SDO, STEREO, NuSTAR, MMS, … • Ground: >40 observatories • Modeling: 7 teams provide predictions of the SC B- connectivity Data distribution: Space- and Ground-based Support Leads PSP E4: Ground-Based Optical Solar Observatories Observatory Location/Time Observations POC Mauna Loa Solar Observatory Big Island of • White light polarization brightness (pB) Joan Burkepile (MLSO) Hawaii, USA • Coronal electron densities 19.5°N • 15s cadence 155.6°W Daily (1700- 0200UT) Big Bear Solar Observatory California, USA • Imaging spectroscopy and polarimetry Wedna Cao (BBSO) Daily • 0.1” resolution Haimin Wang Dunn Solar Telescope New Mexico, • Imaging and spectroscopy at multiple wavelengths Damian Christian USA • IR spectro-polarimetry Jan 15-31 (1500-1700UT) Sayan Solar Obbservatory Russia • Spectrograms and vector magnetograms Misha Demidov 51.6°N 108°E • Coronal obbservations Daily Baikal Astrophysical Russia • Call K Misha Demidov Observatory 54.8°N 105°E • Magnetic Field Daily Kislovodsk Observatory Russia • Full-disk Call K and Halpha (1m cadence) Andrey Tlatov 43.7°N 42.3°E • Photospheric magnetograms2/7/20 Support for PSP Encounter 4 | SPWG Telecon 11 PSP E4: Ground-Based Optical Solar Observatories Observatory Location/Time Observations POC Fuxian Solar Observatory China • High-res 0.3” Halpha images with 11s cadence Zhi Xu 1m NVST telescope 24.6°N 103°E • High-res ~0.1” (after reconstruction) images in the TiO band 0100-0800UT with 30s cadence Huairou Solar Observing China • Halpha Xianyong Bai Station (HSOS) 40.4°N 116.6°E • Photospheric vector magnetic fields 0030-0830UT • Chromospheric LOS magnetic fields ONSET Telescope China Pengfei Chen Istituto Ricerche Solari Locarno, • High-precision polarimetry in the Cal 422.7 nm limb (both limb Renzo Ramelli Locarno (IRSOL) Switzerland and disk) Michele Bianda 46.2°N 8.8°E • Other possible lines include: Na I D1 and D2, He D3, H-alpha, and a C2 molecular band Kanzelhöhe Observatory Austria • Full-disk images in Halpha, Call K, and white light Werner Pötzi 46.7°N 13.9°E • 10 images/minute (4 images/s in flare mode) Daily Hvar Observatory Zagreb, Croatia • Halpha and white light high cadence 2s images Jasa Calogovic 43.2°N 16.5°E • FOV 7 and 11 arcmin, 1” spatial resolution 0600-1300UT 2/7/20 Support for PSP Encounter 4 | SPWG Telecon 12 PSP E4: Ground-Based Optical Solar Observatories Observatory Location/Time Observations POC Astronomical Observatory of Monte Porzio • Full-disk Call K, G-band, res and blue cont. Ilaria Ermolli Rome (PSPT) Catone, Rome, • ~2” resolution, 0.1% pixel-to-pixel precision Italy Catania Solar Observatory Catania, Sicily, • Full-disk images in Halpha and cont at 656nm Paolo Romano Italy • 2” spatial resolution 37.5°N 15.1°E • 1m cadence in campaign mode Pic du Midi Pyrenees, FR • Coronagraphic observations in Halpha and Hel, possibly in Fe Frederic Pitout 42.9°N 0.1°E XII 1074 nm Arturo Lopez Ariste Meudon Observatory France • Full disk Halpha Jean-Marie Malherbe 48.8°N 2.3°E Daily NSO/GONG Netword Multiple • High-sensitivity magnetograms, velocity and intensity images at Alexei Pevtsov locations 1m cadence ~90% duty • Near-real-time seismic images of the farside cycle • Halpha images at 20s cadence Mitaka Observatory Japan • Full-disk Halpha, G-band, Call K, cont. Yoichiro Hanaoka • Halpha velocity maps • Full-disk magnetograms in He 10830Å, Si 10827Å, and Fe 15648Å 2/7/20 Support for PSP Encounter 4 | SPWG Telecon 13 PSP E4: Ground-Based Optical Solar Observatories Observatory Location/Time Observations POC Hida Observatory Japan • Full-disk Halpha images Kiyoshi Ichimoto Félix Aguilar Observatory Argentina • Full-disk H-alpha center line with a 1m cadence Carlos Francile 31.8°S 69.3°W • 30 THz camera (70% of the disk) with 1s cadence Latin America Giant Marambio, • Cosmic rays 2-100 GeV Sergio Dasso Observaory (LAGO)/NEWRUS Antartica 64°S 57°W (etc) Crimean Astrophysical Crimea • Monochromatic and spectral images Valentina Abramenko Observatory (CrAO) 2/7/20 Support for PSP Encounter 4 | SPWG Telecon 14 PSP E4: Ground-Based Radio Solar Observatories Observatory Location/Time Observations POC Arecibo Mike Sulzer [email protected] Expanded Owens Walley California, USA • Microwave spectra and iMaging 1-18GHz Dale Gary Solar Array (EOVSA) Daily (1600- • Full-disk iMages 1/day at 6 frequency bands Sherry Chhabbra 2400UT) • Full-Sun-integrated spectrograMs, 1s cadence Bin Chen Very Large Array (VLA) New Mexico, • Imaging at 1-2 GHz & 230-470 MHz TiM Bastian USA Jan 28, 30, 31 (TBC) Jan 27 • Full-disk Mosaic L & S band Stephen White Long Wavelength Array New Mexico, • 20-80 MHz spectroscopy Stephen White (LWA) USA Jan 27-30 (TBC) NobeyaMa Radioheliograph Japan • Full-disk iMages at 17 and 34 GHz Satoshi Masuda 2300-0600 UT Kislovodsk Observatory Russia • Radio observations at 3 and 5cM Andrey Tlatov 43.7°N 42.3°E MeerKAT South Africa Du Toit 2/7/20 SupportJaMes for PSP Chibueze Encounter 4 | SPWG Telecon 15 PSP E4: Ground-Based Radio Solar Observatories Observatory Location/Time Observations POC Siberian Radioheliograph Siberia, Russia • Full-disk images at 16 or 32 bands in 4-8 GHz range Maria Globa 51.8°N 103°E Alexander Altyntsev Daily 0200- Sergey Lesovoi 0800UT Huairou Solar Radio China Baolin Tan Spectrograph Low-Frequency Array (LOFAR) Netherlands • Solar imaging range 20-70MHz Richard Fallows • High-res solar dynamic spectra 10-77MHz and 110-190MHz Pietro Zucca Murchison Widefield Array Austrailia • Imaging spectroscopy at 24 bands 80-240 MHz Divya Oberoi • 0.5s and 40 kHz resolution Sardinia Radio Telescope San Basilio, • Full-disk solar images at 18 and 26 GHz Alberto Pellizzoni (SRT) Sardinia, Italy • ~50” arcsec angular res 39.5°N 9.2°E Jan 28 0800- 1500UT Nançay Decameter Array France • 10-100 MHz daily spectrograms of the Sun and Jupiter at Sophie Masson 47.4°N 2.2°E various cadences (<1s) and spectral resolutions (<175 kHz) Laurent Lamy Daily 2/7/20 Support for PSP Encounter 4 | SPWG Telecon 16 PSP E4: Ground-based Geospace Observatories Observatory/Satellite Observing Observations POC Mission Window PFISR Continuous • IPY27 (1% duty cycle): 4 beams, long pulse (F-region) and Roger Varney (low duty cycle) alternating codes (E-region) [email protected] • Themis36: 23 beams, long pulse (F-region) and alternating codes (E-region) • MSWinds26 (For ELFIN): 4 beams, barker codes (D-region), alternating codes (E-region), and long pulse (F-region) • WorldDay35: 11 beams, long pulse (F-region) and alternating codes (E-region) Calendar: data.amisr.com/database/61/sched/2020/01/ RISR-N Continuous • LowDuty2 (3.5% duty cycle): 5 beams long pulse (F-region) and Roger