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Glows cdf attrs update #725

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merged 11 commits into from
Aug 9, 2024
Merged

Glows cdf attrs update #725

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c647183
first pass
maxinelasp Jul 29, 2024
f7c0688
MS mods
anamanica Jul 30, 2024
3ce2ada
Glows MS CDF attrs update
anamanica Jul 30, 2024
bcda5fc
Fixing tests
anamanica Jul 30, 2024
e65e4e2
Updating Branch
anamanica Aug 7, 2024
0483be4
Updating Branch
anamanica Aug 7, 2024
635235a
Using default epoch
anamanica Aug 8, 2024
e831421
All PR comments gone through
anamanica Aug 8, 2024
e457d73
Updating Branch
anamanica Aug 8, 2024
5706529
Updating branch.
anamanica Aug 9, 2024
652075d
Depend_1 attr change
anamanica Aug 9, 2024
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13 changes: 7 additions & 6 deletions imap_processing/cdf/config/imap_glows_global_cdf_attrs.yaml
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Expand Up @@ -2,14 +2,15 @@ instrument_base: &instrument_base
Descriptor: GLOWS>GLObal Solar Wind Structure
TEXT: >
The GLObal Solar Wind Structure (GLOWS) is a non-imaging single-pixel Lyman-alpha
photometer that will be used to observe the sky distribution of the helioglow to
better understand the evolution of the solar wind structure.
The Lyman-alpha photon counts from these observations can be used to build a more
comprehensive picture of the solar wind structure and how it changes through the
solar cycles.
photometer to investigate the global heliolatitudinal structure of the solar wind
and its evolution during the solar cycle. Additionally, GLOWS investigates the
distribution of interstellar neutral hydrogen (ISN H) and the solar radiation
pressure acting on ISN H. The objectives of GLOWS are accomplished by observation
of the modulation of heliospheric backscatter glow of ISN H (the helioglow)
along a scanning circle in the sky.
GLOWS design and assembly is led by the Space Research Center, Warsaw, Poland
(CBK PAN). See https://imap.princeton.edu/instruments/glows for more details.
Instrument_type: Particles (space)
Instrument_type: Imagers (space)

imap_glows_l1a_hist:
<<: *instrument_base
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