RHESSI_data_analysis

rhessi_data_analysis@solar.physics.montana.edu

32 discussions

2024 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 23 Jul '24

23 Jul '24

Dear colleagues, There is just over week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the 7th (!) annual installment of our session for next-generation missions, instruments, technology, and science studying high-energy processes on the Sun. This includes theory/modeling to drive new measurements/missions! We welcome a broad range of topics on missions, mission concepts, enabling technology, new measurements/data, driving theories and models ... and especially encourage an eye for medium- and long-term outlook. Deadline to submit is 11:59pm EDT on July 31 (next Wednesday). Session/submission link and description are below, for your reference. We look forward to your exciting submissions! https://agu.confex.com/agu/agu24/prelim.cgi/Session/227061 SH016 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; SolO; MinXSS; SphinX; Chandrayaan-2; the FOXSI, MaGIXS, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories including NuSTAR, Fermi, ALMA, and VLA; have significantly advanced our understanding of these phenomena. They have also highlighted the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot/non-thermal) aspects of the Sun, and the science enabled by such new observations. --- Amir Caspi, on behalf of Chris Moore, Julie Vievering, P.S. Athiray, Milo Buitrago-Casas

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Re: 2023 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 01 Aug '23

01 Aug '23

Dear colleagues, A gentle reminder that there is just one day left to submit abstracts to AGU (due tomorrow, Weds, Aug 2 at 11:59pm ET). We hope you'll consider session SH011, details below. =) Thanks! --- Amir On 07/26/2023, 9:57 AM, "Amir Caspi" <amir(a)boulder.swri.edu> wrote: Dear colleagues, There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the 6th (!) annual installment of our session for next-generation missions, instruments, technology, and science studying high-energy processes on the Sun. This includes theory/modeling to drive new measurements/missions! We welcome a broad range of topics on missions, mission concepts, enabling technology, new measurements/data, driving theories and models ... and especially encourage an eye for medium- and long-term outlook. Deadline to submit is 11:59pm EDT on Aug 2nd (next Wednesday). Session/submission link and description are below, for your reference. We look forward to your exciting submissions! https://agu.confex.com/agu/fm23/prelim.cgi/Session/188319 SH011 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; SolO; MinXSS; SphinX; Chandrayaan-2; the FOXSI, MaGIXS, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories including NuSTAR, Fermi, ALMA, and VLA; have significantly advanced our understanding of these phenomena. They have also highlighted the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot/non-thermal) aspects of the Sun, and the science enabled by such new observations. --- Amir Caspi, on behalf of Chris Moore, Julie Vievering, P.S. Athiray, Shaheda Begum Shaik

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2023 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 26 Jul '23

26 Jul '23

Dear colleagues, There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the 6th (!) annual installment of our session for next-generation missions, instruments, technology, and science studying high-energy processes on the Sun. This includes theory/modeling to drive new measurements/missions! We welcome a broad range of topics on missions, mission concepts, enabling technology, new measurements/data, driving theories and models ... and especially encourage an eye for medium- and long-term outlook. Deadline to submit is 11:59pm EDT on Aug 2nd (next Wednesday). Session/submission link and description are below, for your reference. We look forward to your exciting submissions! https://agu.confex.com/agu/fm23/prelim.cgi/Session/188319 SH011 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; SolO; MinXSS; SphinX; Chandrayaan-2; the FOXSI, MaGIXS, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories including NuSTAR, Fermi, ALMA, and VLA; have significantly advanced our understanding of these phenomena. They have also highlighted the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot/non-thermal) aspects of the Sun, and the science enabled by such new observations. --- Amir Caspi, on behalf of Chris Moore, Julie Vievering, P.S. Athiray, Shaheda Begum Shaik

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Solar Physics High Energy Research (SPHERE) Workshop — 11–15 July 2022 — Boulder, CO, USA + Windisch, CH + online
by Amir Caspi 04 Apr '23

04 Apr '23

Dear colleagues, The Solar Physics High Energy Research (SPHERE) Workshop -- formerly known as the RHESSI workshop, and now motivated by SolO/STIX, MinXSS, EOVSA, and many other current and upcoming missions -- will be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland. The workshop agenda will include plenary topical sessions, held jointly between all locations, featuring invited talks and facilitated, open discussions on targeted science questions. This interactive format is intended to foster both broader and deeper collaboration and understanding amongst our community, to propel progress and enhance success by breaking down silos both within the high-energy solar physics and among solar and space physics in general. Additional independent morning (EU) and afternoon (US) sessions will feature tutorials, posters, early-career talks, and open collaboration. Registration is required, and U.S. hotel accommodations (for the contract hotel) will be handled through the registration form. Abstracts for posters and early-career presentations, and suggestions for open topical discussions, will be solicited soon. The workshop website at https://sphere.boulder.swri.edu is operational with preliminary information, including travel information, and will be updated soon with registration information and deadlines. We hope to see you soon in Boulder, Windisch, or online! – Amir Caspi & Säm Krucker, on behalf of the organizing committee

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COMPLETE white paper -- invitation to co-sign (last-minute!)
by Amir Caspi 07 Sep '22

07 Sep '22

Hi all, Sorry that this is VERY last minute. Please forward this on to anyone whom you feel would be interested. You are all invited to co-sign three white papers related to COMPLETE, a flagship mission concept for 3D understanding of magnetic energy storage and release in the corona. Papers are linked and briefly described below -- the mission and science papers still need some polish which we'll be doing today, but should hopefully be sufficient for your evaluation. Please add your name to the respective author spreadsheets by 6pm MDT if you would like to co-sign! Science: describing the need for comprehensive 3D understanding of coronal magnetic energy storage and release. Paper draft -- https://drive.google.com/file/d/1GW72bPuDGbkAXRbXovvz9PMLExy7jORT/view?usp=… Author list -- https://docs.google.com/spreadsheets/d/1GZMhei9RIsp7ra_osGkhAnzAWjWg3Rn2/ed… Mission: describing the COMPLETE concept, brief science overview, instrumentation, mission, and timeline/cost Paper draft -- https://drive.google.com/file/d/1GTLuV6eAB6XAZmXlAaoDWz20_pOmprsq/view?usp=… Author list -- https://docs.google.com/spreadsheets/d/1GevUH2qjGHyL8-U3IpVAkSAmdOanVQOV/ed… Data philosophy: describing the need for unified data formats, and new assimilation and analysis frameworks ... uses COMPLETE as a case study but extends well beyond COMPLETE! Paper (final) -- https://www.overleaf.com/3429236955tpwhmdcfkkbm Author list -- https://docs.google.com/spreadsheets/d/1ACZ6cUi139b6h1YWKynhWCc7rIJ53KLG/ed… We welcome your support! --- Amir

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Registration/abstracts closing soon — Solar Physics High Energy Research (SPHERE) Workshop — 11–15 July 2022 — Boulder/Windisch/online
by Amir Caspi 15 Jun '22

15 Jun '22

Dear colleagues, Registration and abstract submission are CLOSING SOON for the Solar Physics High Energy Research (SPHERE) Workshop, to be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland. For full details, please visit the workshop website: https://sphere.boulder.swri.edu Abstract submission deadline: 17 June 2022 NOTE: please contact the organizers if you will have trouble meeting this deadline and need additional time. The complete schedule/agenda will be posted ASAP, before the end of June. Registration deadlines: U.S. – 30 June 2022 | Europe – 11 July 2022 | virtual – 11 July 2022 Registration fee: none U.S. hotel reservation deadline: 30 June 2022 (through the registration form) Oral presentation requests will be accepted from early-career researchers (up to 5 years post PhD) and students only – the ongoing pandemic has severely restricted opportunities for young researchers, so we are prioritizing oral presentations for them. Poster presentations will be accepted from any attendee. Because of the hybrid format, posters must be submitted as PDF for online access, and may also be presented in person (format TBD). We hope to see you soon in Boulder, Windisch, or online! – Amir Caspi & Säm Krucker, on behalf of the organizing committee

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Registration/abstracts open — Solar Physics High Energy Research (SPHERE) Workshop — 11–15 July 2022 — Boulder/Windisch/online
by Amir Caspi 01 Jun '22

01 Jun '22

Dear colleagues, Registration and abstract submission is NOW OPEN for the Solar Physics High Energy Research (SPHERE) Workshop, to be held 11–15 July 2022. The workshop will be a hybrid format with online access and two in-person locations: Southwest Research Institute (SwRI) in Boulder, Colorado, USA and Fachhochschule Nordwestschweiz (FHNW) in Windisch, Switzerland. For full details, please visit the workshop website: https://sphere.boulder.swri.edu Registration deadline: U.S. – 30th June 2022 | Europe – 11th July 2022 Registration fee: none U.S. hotel reservation deadline: 30th June 2022 (through the registration form) Abstract submission deadline: 17th June 2022 NOTE: Please contact the organizers if you will have trouble meeting the abstract deadline and need additional time Oral presentation requests will be accepted from early-career researchers (up to 5 years post-PhD) and students only – the ongoing pandemic has severely restricted opportunities for young researchers, so we are prioritizing oral presentations for them. Poster presentations will be accepted from any attendee. Because of the hybrid format, posters must be submitted as PDF for online access, and may also be presented in person (format TBD). We hope to see you soon in Boulder, Windisch, or online! – Amir Caspi & Säm Krucker, on behalf of the organizing committee

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TESS session 16: next-gen missions -- call for abstracts
by Amir Caspi 13 Apr '22

13 Apr '22

Hi all, It's a bit last-minute, but I wanted to ensure that everyone knew about our TESS session #16, "High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond." This is the next installment in our now long-running successful series of AGU sessions for next-gen missions, instruments, technology, and science studying high-energy processes on the Sun. Please consider submitting an abstract to the session! We welcome a broad range of topics, and especially encourage decadal concepts and long-term outlook. Abstracts are due this Friday, April 15. The session description is below, for your reference. Abstracts can be submitted at the following URL: https://submissions.mirasmart.com/TESS2022/Splash.aspx Looking forward to seeing you at TESS, in session 16! =) --- Amir, on behalf of the conveners 16. Title: High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Conveners: Amir Caspi (SwRI), Lindsay Glesener (UMN), Tom Woods (CU/LASP) Description: Energetic phenomena on the Sun, including impulsively-driven eruptions (flares and coronal mass ejections) and more gradual coronal heating and solar wind outflows, provide crucial insight into unique regimes of plasma physics and astrophysical processes, and are also the primary drivers of space weather. Physical processes within these phenomena, including particle acceleration and plasma heating, emit signatures across the electromagnetic spectrum, from Xrays/gamma-rays, through UV/EUV, to infrared and radio. Spectral and imaging observations of these emissions provide critical diagnostics into the macro- and microphysics underlying these processes. The X-ray and EUV emissions are also significantly geoeffective, contributing to societally-important dynamical effects in Earth’s upper atmosphere and ionosphere on a variety of timescales. Recent measurements from numerous solar observatories including RHESSI; SDO; SolO; MinXSS; SphinX; Chandrayaan-2; the FOXSI, MaGIXS, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others – and from opportunistic observations by non-solar observatories such as NuSTAR, Fermi, ALMA, and VLA – have significantly advanced our understanding of these phenomena and their driving processes. They have also shown the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes and the solar magnetic field that powers them. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot and non-thermal) aspects of the Sun, as well as the solar magnetic field. Presentations are also invited on the science enabled by such new observations, including space weather-related science and impacts to Earth’s atmosphere and ionosphere. Recognizing the 2023-2032 Heliophysics Decadal Survey currently under way and the community-led Heliophysics 2050 vision, we also encourage presentations that include longer-term future outlooks and both intra- and inter-disciplinary integration of solar and heliospheric physics, space physics, and other relevant fields.

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LAST CALL: 2021 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 03 Aug '21

03 Aug '21

Dear colleagues, A reminder that AGU abstracts are due tomorrow -- Wednesday, Aug 4 -- at 11:59pm EDT. If you have not yet done so, please consider submitting to our next-generation solar session, SH017. Any and all submissions are welcome, and I am happy to answer questions if you have any. Details and link are below. Cheers! --- Amir On 07/27/2021, 10:42 AM, "Amir Caspi" <amir(a)boulder.swri.edu> wrote: Dear colleagues, There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the fourth-annual installment of our session for next-generation remote-sensing missions. Like last year, this year the focus includes all remote sensing, including imaging, spectroscopy, polarimetry, and combinations of those, plus anything else I'm missing. Given the imminent Decadal Survey, we encourage submissions with an eye both for near-term _and_ long-term (decadal or beyond) timescales for development. Session link and description are below. Deadline is 11:59pm EDT on Aug 4th (next Wednesday). We look forward to your exciting submissions! https://agu.confex.com/agu/fm21/prelim.cgi/Session/121896 SH017 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; MinXSS; SphinX; the FOXSI, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories such as NuSTAR, Fermi, ALMA, and VLA, have significantly advanced our understanding of these phenomena. They have also shown the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot and non-thermal) aspects of the Sun, and the science enabled by such new observations. --- Amir Caspi, Lindsay Glesener, Jenna Samra, & Athiray Panchapakesan

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2021 AGU Session on high-energy solar remote-sensing missions/instruments
by Amir Caspi 27 Jul '21

27 Jul '21

Dear colleagues, There is one week left to submit abstracts to this year's AGU Fall Meeting, a hybrid meeting with both in-person and virtual components. We invite you to submit an abstract to the fourth-annual installment of our session for next-generation remote-sensing missions. Like last year, this year the focus includes all remote sensing, including imaging, spectroscopy, polarimetry, and combinations of those, plus anything else I'm missing. Given the imminent Decadal Survey, we encourage submissions with an eye both for near-term _and_ long-term (decadal or beyond) timescales for development. Session link and description are below. Deadline is 11:59pm EDT on Aug 4th (next Wednesday). We look forward to your exciting submissions! https://agu.confex.com/agu/fm21/prelim.cgi/Session/121896 SH017 - High-Energy Solar Investigations Through Next-Generation Remote Sensing: Spectroscopy, Imaging, and Beyond Energetic processes on the Sun, including particle acceleration and plasma heating during flares and quiescence, emit signatures across the electromagnetic spectrum, from X-rays/gamma-rays, through UV/EUV, to infrared and radio. Recent measurements from numerous solar observatories including RHESSI; SDO; MinXSS; SphinX; the FOXSI, Hi-C, EUNIS, and EVE rockets; the GRIPS balloon; EOVSA; and many others; and from opportunistic observations by non-solar observatories such as NuSTAR, Fermi, ALMA, and VLA, have significantly advanced our understanding of these phenomena. They have also shown the pressing need for increasingly advanced high-resolution, high-sensitivity measurements across the entire spectrum, including polarimetry and especially imaging spectroscopy, to gain further insight into these high-energy processes. This session invites presentations covering new instrumentation, enabling technology, missions, and concepts for next-generation solar remote sensing -- including spectroscopy, imaging, and beyond -- aimed at studying high-energy (hot and non-thermal) aspects of the Sun, and the science enabled by such new observations. --- Amir Caspi, Lindsay Glesener, Jenna Samra, & Athiray Panchapakesan

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RHESSI_data_analysis