Search
Close this search box.

Meet the “Scene Select Mechanism”—Part of the LDCM Thermal Infrared Sensor

Meet the “Scene Select Mechanism”—Part of the LDCM Thermal Infrared Sensor

Special Topics: LDCM and LDCM Components

Engineer (in a "bunny suit") working on the Scene Select Mechanism of the Thermal Infrared Sensor (TIRS) that will fly on LDCM.
Engineer (in a “bunny suit”) working on the Scene Select Mechanism of the Thermal Infrared Sensor (TIRS) that will fly on LDCM.

The Scene Select Mechanism is an apparatus that rotates the LDCM Thermal Infrared Sensor (TIRS) mirror among three scenes: the Earth view (“nadir;” when imaging the Earth), and two calibration views (one of a warm blackbody carried onboard and the other of a deep-space cold view). The Earth view requirements for instrument pointing are very stringent, correct image positioning depends on precise pointing and that position must be returned to faithfully after each calibration sequence. The requirement for the Thermal Infrared Sensor (TIRS) is to image up to 44 minutes continuously, which corresponds to the longest uninterrupted landmass pass that TIRS needs to image before traveling over water—when the calibration sequence can be performed again. (This long-land path curves from Northern Russia to the southern tip of Africa.)
Bunny suit: The TIRS instrument is kept in a cleanroom and anyone working on it must wear cleanroom clothing that minimizes particulates coming from a person’s clothing. Prior to entering the cleanroom, each person also takes an “air shower” which blows any excess dust off of them before entering the cleanroom. Inside the Class 10,000 cleanroom are filters which continuously filter the air inside to ensure there are no more than 10,000 particles greater than 0.5 microns in size within a cubic foot of air (the average home has about 300,000 particles per cubic foot).

On Key

Recent Posts

STELLA Photos

STELLA Spring Webinar: April 15, 2024

STELLA users will talk about their experiences using the DIY spectrometer during this webinar. Panelists include Bianca Cilento (RIT), Karen Karker (SUNY), and Peder Nelson (OSU and NASA GLOBE Observer).

Read More »
On Key

Related Posts

STELLA Photos

STELLA Spring Webinar: April 15, 2024

STELLA users will talk about their experiences using the DIY spectrometer during this webinar. Panelists include Bianca Cilento (RIT), Karen Karker (SUNY), and Peder Nelson (OSU and NASA GLOBE Observer).

Read More »