Lectures2 Flashcards

EOS Terra

1
Q

Terra instruments

A

 ASTER (Advanced Spaceborne Thermal Artists impression of Spot 5
Emission and Reflection Radiometer)
 CERES (Clouds and the Earth’s Radiant Energy System)
 MISR (Multi-angle Imaging Spectro- Radiometer)
 MODIS (Moderate-resolution Imaging Spectroradiometer)
 MOPPIT (Measurements of Pollution in the Troposphere)

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2
Q

ASTER main functions

A

detailed maps of land surface
temperature, emissivity, reflectance,
and elevation

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3
Q

CERES manin function

A

radiation bodies, when emitted. Radiation is important because main driver for climate.

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4
Q

MOPPIT

A

knowledge of knowledge of lower atmosphere, measurements of pollution in the troposphere. focus on distribution, transport, and sinks of CO and methane in troposphere.

Gas correlation spectroscopy. 3 spectral bands, two for CO and one for CH4.

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5
Q

CO concentration can be caused by

A

biomass burning–fires

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6
Q

MISR main function

A

Multi-angle Imagingin spectro-radiometer

9 widely spaced angles
ongoing global coverage with high spatial detail.

multiple angles also comparison between different levels of radiation reflected at different angles. Need to know the amount of sunlights that is scattered in different direction under natural conditions. Important for radiation and energy budget.

Aerosols / clouds=reflected right back.

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7
Q

MISR bands

A

4 bands -vis +NIR

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8
Q

SO4

A

sulfate

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9
Q

MISR main goals

A

Aerosols:
abundance and type
impact on climate

Surface:
Land cover type,
directional / hemispherical reflectances
biosphere / atmopshere interactions

Clouds:
cloud screening
classification–type and alititude
impact on climate

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10
Q

MISR: scattering angle

A

is the angle between the sun’s direction and viewing direction

Most of what can be learned about cloud/dust /surface comes from studying from different angles

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11
Q

MODIS

A

important instrument on Terra / Aqua

2330-km swath

every point on world every 1-2 days in 36 discrete bands (reflected and emitted radiation)

improves on AVHRR (similar size track), tracks wider array of earth’s “vital signs” than any other Terra sensor

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12
Q

MODIS spectral bands

A

see table

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13
Q

Ocean color sensors

A

Seawifs, CZSwhatever, MODIS

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14
Q

For cloud vapor

A

5-8 micrometers is atmospheric window for thermal, but can be used for cloud vapor (see 6-7 in MODIS table)

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15
Q

find data here

A

usgs , echo reverb (nasa)

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16
Q

CERES: Clouds and Energy Cycle

A

see graphic

Plus All previous tables with EOS sensors tables….

17
Q

radiation budget

A

Net = incoming = outgoing
R* (or Q*)= K(in) - K (out) + L(in) - L(out)

Thus R* = K* + L*

K= shortwave
L = longwave (thermal)

For albedo = K(in) [1-alpha (albedo)]

Q(energy budget) = Qh + Qe + Qg
h=sensible heat, e=latent heat, g=ground flux