9
SORCE Sonoma meeting • XPS • TIM • SIM • SOLSTICE

SORCE Sonoma meeting XPS TIM SIM SOLSTICE. XP#FilterBand 1Band 2 1Ti/C0.1-7 nm- 2Ti/C0.1-7 nm- 3Al/Sc/C0.1-3 nm17-23 nm 4BareVis- 5Al/Nb/C0.1-3 nm17-21

  • View
    218

  • Download
    1

Embed Size (px)

Citation preview

SORCE Sonoma meeting

• XPS

• TIM

• SIM

• SOLSTICE

XP# Filter Band 1 Band 2

1 Ti/C 0.1-7 nm -

2 Ti/C 0.1-7 nm -

3 Al/Sc/C 0.1-3 nm 17-23 nm

4 Bare Vis -

5 Al/Nb/C 0.1-3 nm 17-21 nm

6 Ti/Mo/Au 0.1-11 nm

7 Ti/Mo/Si 0.1-3 nm 11-17 nm

8 Bare Vis -

9 Al/Cr 0.1-7 nm 29-34 nm

10 Al/Mn 0.1-7 nm 25-34 nm

11 Lyman- 121-122 -

12 Bare Vis -

SORCE XPS: an array of Si diodes

SORCE XPS is almost identical to TIMED SEE XPS that began measurements in January 2002.

Responsivity available @ http://lasp.colorado.edu/see/see_xps.htmlin the form of IDL save files and a reader program

Flare

Type

SORCE Mission

May 26 - June 26

Oct. 19 - Nov. 4

Large > x4 30 9 13

Total > 3- 195 84 83

TIM sees “dips”

Conclusions

• SORCE (and TIMED) have lots of flare data

• The data are well-calibrated and available

• The SORCE team needs instruction on keV

• The first total-irradiance flare observations

• The first complete XUVO flare data, including Ly-