Skip to main content

ESA Data Ontology

Search from vocabulary

Content language

Concept information

Instruments > Solar/Space Observing Instruments > Ultraviolet Instruments > Thermal Radiation Experiment

Preferred term

Thermal Radiation Experiment  

Definition

  • The Explorer 7 thermal radiation experiment was designed to measure incident and reflected solar UV radiation and terrestrial IR radiation in order to obtain a better understanding of the driving forces of the earth-atmosphere system. The primary instrumentation consisted of five bolometers in the form of hollow silver hemispheres that were thermally insulated from, but in close proximity to specially aluminized mirrors. The hemispheres thereby behaved very much like isolated spheres in space. Two of the hemispheres had black coatings and responded about equally to solar and terrestrial radiation. A third hemisphere, coated white, was more sensitive to terrestrial radiation than to solar radiation. A fourth, which had a gold metal surface, was more sensitive to solar radiation than to terrestrial radiation. The fifth hemisphere, protected from direct sunlight, was used to measure the reflected sunlight. A glass-coated bead thermistor was mounted on the top of each hemisphere to measure the temperature. A complete set of four temperature observations and one reference sample required 30 s. Thus, in each orbit, about 180 temperature measurements could be obtained. The experiment was a success, and usable data were obtained from launch until February 28, 1961. (en)

Broader concept

Change note

  • 2021-08-16 10:52:57.0 [tstevens] Insert Concept add broader relation (Thermal Radiation Experiment [5475ab0a-4c92-495d-a071-b86b6e7df49f,706580] - Ultraviolet Instruments [b5e4912d-3224-4d7b-924c-a697677775c6,698985]);
  • 2021-08-16 10:53:29.0 [tstevens] insert Definition (id: null text: The Explorer 7 thermal radiation experiment was designed to measure incident and reflected solar UV radiation and terrestrial IR radiation in order to obtain a better understanding of the driving forces of the earth-atmosphere system. The primary instrumentation consisted of five bolometers in the form of hollow silver hemispheres that were thermally insulated from, but in close proximity to specially aluminized mirrors. The hemispheres thereby behaved very much like isolated spheres in space. Two of the hemispheres had black coatings and responded about equally to solar and terrestrial radiation. A third hemisphere, coated white, was more sensitive to terrestrial radiation than to solar radiation. A fourth, which had a gold metal surface, was more sensitive to solar radiation than to terrestrial radiation. The fifth hemisphere, protected from direct sunlight, was used to measure the reflected sunlight. A glass-coated bead thermistor was mounted on the top of each hemisphere to measure the temperature. A complete set of four temperature observations and one reference sample required 30 s. Thus, in each orbit, about 180 temperature measurements could be obtained. The experiment was a success, and usable data were obtained from launch until February 28, 1961. language code: en);

URI

https://gcmd.earthdata.nasa.gov/kms/concept/5475ab0a-4c92-495d-a071-b86b6e7df49f

Download this concept:

RDF/XML TURTLE JSON-LD Last modified 12/6/20