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The overarching goal of this workshop is to come to an understanding of how the EUV irradiance is being measured and to develop a unified strategy for determining the absolute value of the EUV irradiance and how it varies, both in wavelength and time.
Kickoff/Keynote talk on "Lessons “Lessons Learned from TSI Inter-Comparisons" Comparisons” by Greg Kopp.
Logistics
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Detailed Agenda
Tuesday Oct. 25
8:00 - 8:30 a.m. Continental Breakfast (provided at LASP)
Session 1: Introductions
8:30 - 9:00 a.m. Welcome Andrew Jones
9:00 - 9:30 a.m. Workshop Purpose Frank Eparvier
9:30 - 10:15 a.m. Keynote: TSI Comparisons - Lessons Learned Greg Kopp
10:15 - 10:45 a.m. Break (Coffee provided)
10:45 - 11:15 a.m. Comparisons - The Devil is in the Details Frank Eparvier
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11:15 - 11:25 a.m. Instrument Overview Andrew Jones
Photometers
11:25 - 11:45 a.m. SEE and SORCE XPS Tom Woods
11:45 - 12:05 p.m. LYRA Marie Dominique
12:05 - 12:15 p.m. Discussion
12:15 - 1:00 p.m. Lunch (provided at LASP)
General Talks: Why it Matters
1:00 - 1:20 p.m. Solar Physics Rachel Hock
1:20 - 1:40 p.m. Application of EUV Measurements for the Derivation of Parameters for the Interstellar Gas Flow through the Heliosphere Peter Bochsler and Eberhard Möbius
1:40 - 1:50 p.m. Discussion
Spectrophotometers
1:50 - 2:05 p.m. SoHO-SEM Seth Weiman
2:05 - 2:20 p.m. SDO-EVE-ESP Leonid Didkovsky
2:20 - 2:40 p.m. GOES-NOP-EUV Slides presented by Jones
2:40 - 2:50 p.m. Discussion
2:50 - 3:20 p.m. Break (Coffee Provided)
Spectrometers & Spectrographs
3:20 - 3:40 p.m. TIMED-SEE-EGS Frank Eparvier
3:40 - 4:00 p.m. SDO-EVE-MEGS Tom Woods
4:20 - 4:35 p.m. SoHO-CDS Instrument , Calibration Slides presented by Jones
4:35 - 4:45 p.m. Discussion
4:45 - 5:00 p.m. Day 1 Wrap-up and Homework Assignments
6:30 p.m. Group Dinner --- Walnut Brewery, 1123 Walnut Street, Boulder, CO 80302-5116
Reservation under the name "Solar",www.walnutbrewery.com
Wednesday Oct. 26
8:00 - 8:30 a.m. Continental Breakfast (provided at LASP)
General Talks: Calibration Facilities
8:30 - 8:50 a.m. NIST Uwe Arp
8:50 - 9:10 a.m. NSLS Jim Bremer (Jim's Zone Plate Presentation )
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9:10 - 9:30 a.m. SEE and SORCE XPS Tom Woods
9:30 - 9:50 a.m. LYRA Ingolf Dammasch
9:50 - 10:10 a.m. SoHO SEM Seth Weiman
10:10 - 10:30 a.m. SDO-EVE-ESP Leonid Didkovsky
10:30 - 10:50 a.m. Break (Coffee provided)
10:50 - 11:10 a.m. GOES-NOP-EUV Slides presented by Jones
11:10 - 11:30 a.m. TIMED-SEE-EGS Frank Eparvier
11:30 - 11:50 a.m. SDO-EVE-MEGS Tom Woods
11:50 - 12:10 p.m. SOLACES Instrument , (animation ) -Raimund Brunner, Calibration -Bernd Nikutowski
12:30 - 1:15 p.m. Lunch (provided at LASP)
1:15 - 1:45 p.m. Tour of LASP
Session 4: Data Comparison Splinters
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- ESP Bandpasses
- May 15 2010, March 4 2011, 0-7, 17-23, 26-34, 121.6 nm comparisons
Working Dinner (if necessary/desired we will order food to be delivered to LASP)
Thursday Oct. 27
8:00 - 8:30 a.m. Continental Breakfast (provided at LASP)
General Talks: Empirical Models
8:30 - 8:50 a.m. FISM and the TIMED-SEE Record Phil Chamberlin
8:50 - 9:10 a.m. Discussion
9:10 - 10:20 a.m. Splinter Group Reports PDF of Comparison Table
10:20 - 10:50 a.m. Break (Coffee provided)
10:50 - 12:00 noon Discussion -- What next? Future plans?
12:00 - 12:15 p.m. Workshop Wrap-up / Summary
12:15 - 1:00 p.m. Lunch -- Box lunches provided (to go or stay) Move to SPSC Building
1:00 - 5:00 p.m. Continued discussion for those staying in SPSC Building
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