Data · collection
SOHO/Charge, Element, and Isotope Analysis System (CELIAS) Data Archive
Listed in NASA Earthdata CMR
The CELIAS instrument is designed to study the composition of the solar wind (SW) and of solar and interplanetary energetic particles on SOHO.
Description
SOHO is a project of international cooperation between ESA and NASA. The CELIAS instrument consists of three different sensors with associated electronics, which are optimized each for a particular aspect of ion composition.
These aspects are the elemental, isotopic, and ionic charge composition of SW or energetic ions emanating from the Sun. In addition, the Solar EUV Monitor (SEM) has been included into CELIAS for monitoring the absolute EUV flux from the Sun. Particle abundance observations of the solar wind and of solar energetic particles (SEP) by itself, and in close correlation with optically observable phenomena on the Sun, will allow to tackle basically unsolved questions in solar physics such as: (1) the steady heating process in the corona, (2) SW acceleration processes, (3) dynamic heating phenomena driven by magnetic fields or waves, e.g. heating in coronal mass ejections, filament eruptions, flares, (4) SEP acceleration processes, (5) processes leading to variations in abundances (elemental, ionic charge, isotopic) and (6) the relation between composition and events/regions in the solar atmosphere.
Read the rest (3 more)
Further scientific goals of CELIAS are to study the composition and dynamics of interplanetary pick-up ions in correlation with the solar EUV flux. For this purpose a solar EUV flux monitor (SEM) for the wavelength 17 to 70 nm has been included into the CELIAS instrument as a sub-unit of the STOF sensor. The SEM serves also to monitor the total absolute EUV flux for the large EUV telescopes on SOHO.
Evidently, the understanding of the phenomena outlined above requires collaboration with many other astrophysical disciplines. Among them are ground based observations including radio astronomical data (e.g. the well known Type III kilometric radio bursts which are related to the strong enrichment of certain species in SEP's) or the interpretation of solar wind abundances in terms of solar abundances as derived from photospheric spectra, meteoritic composition, and from solar oscillation data.
All SOHO/CELIAS data are available from the public SOHO data archive: sohowww.nascom.nasa.gov/data/data.html Mirror archives are available at: SOHO Archive at Rutherford Appleton Laboratory, UK.: trace.solararchive.rl.ac.uk/soho/ SOHO Archive at the Institut d'Astrophysique Spatiale, France: idc-medoc.ias.u-psud.fr/ SOHO Archive at Osservatorio Astronomico di Torino, Torino, Italy: solar.to.astro.it/
Links
Get the data
- Access to SOHO archive and CELIAS data sohowww.nascom.nasa.gov/data ↗
download · from NASA CMR
- Access to additional CELIAS data space.unibe.ch/soho/data.html ↗
download · from NASA CMR
- Gallery of CELIAS images space.unibe.ch/soho/gallery.html ↗
download · from NASA CMR
Documentation and papers
- CELIAS Home Page space.unibe.ch/soho ↗
documentation · from NASA CMR
Catalogue records · 2
- CMR record cmr.earthdata.nasa.gov/search/concepts/C1214614573-SCIOPS.html ↗
catalogue entry · from NASA CMR
- CMR UMM-JSON cmr.earthdata.nasa.gov/search/concepts/C1214614573-SCIOPS.umm_json ↗
metadata API · from NASA CMR
Topics
- Stated by source
- Alpha Particle Flux · Charge, Element, and Isotope Analysis System · Electron Flux · Ion Chemistry/Ionization · Ion Flux · Particle Composition · Particle Density · Particle Speed · Particle Temperature · Proton Flux · Solar Active Regions · Solar and Heliospheric Observatory · Solar Flares · Solar Imagery · Solar Ultraviolet Emissions · Solar Wind
Provenance · 1 source records, 22 field assertions
| Source | Key | Last seen | Raw |
|---|---|---|---|
| NASA Earthdata CMR | C1214614573-SCIOPS | 13 d ago | JSON v1 |
| Field | Assertion | Extractor | Evidence |
|---|---|---|---|
| access_level | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[instrument].gcmd_instrument:celias | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/ionosphere-magnetosphere-dynamics/ion-chemistry-ionization | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/ionosphere-magnetosphere-dynamics/solar-wind | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-activity/solar-active-regions | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-activity/solar-flares | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-activity/solar-imagery | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-activity/solar-ultraviolet-emissions | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-flux/alpha-particle-flux | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-flux/electron-flux | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-flux/ion-flux | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-flux/proton-flux | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-properties/particle-composition | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-properties/particle-density | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-properties/particle-speed | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[measured_variable].gcmd:earth-science/sun-earth-interactions/solar-energetic-particle-properties/particle-temperature | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| concepts[platform].gcmd_platform:soho | source · NASA CMR | connector:nasa_cmr@1.0.0 | |
| description | source · NASA CMR | connector:nasa_cmr@1.0.0 | /umm/Abstract |
| spatial | source · NASA CMR | connector:nasa_cmr@1.0.0 | /umm/SpatialExtent |
| temporal | source · NASA CMR | connector:nasa_cmr@1.0.0 | /umm/TemporalExtents |
| title | source · NASA CMR | connector:nasa_cmr@1.0.0 | /umm/EntryTitle |
| version_label | source · NASA CMR | connector:nasa_cmr@1.0.0 |