English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Conference Paper

On the future of Earth radiation and energy imbalance measurements

Authors

Hakuba,  Maria
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Pilewskie,  Peter
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

Stephens,  Graeme
IUGG 2023, General Assemblies, 1 General, International Union of Geodesy and Geophysics (IUGG), External Organizations;

External Ressource
No external resources are shared
Fulltext (public)
There are no public fulltexts stored in GFZpublic
Supplementary Material (public)
There is no public supplementary material available
Citation

Hakuba, M., Pilewskie, P., Stephens, G. (2023): On the future of Earth radiation and energy imbalance measurements, XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG) (Berlin 2023).
https://doi.org/10.57757/IUGG23-4826


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5021231
Abstract
The upcoming Libera mission, NASA’s first Earth Venture Continuity selection, will provide seamless continuity to current broadband radiance measurements obtained by the Clouds and Earth’s Radiant Energy System (CERES) project since March 2000. Leveraging advanced detector technologies, Libera will measure the broadband total, longwave, and shortwave radiances akin to CERES and carry a fourth radiometer to measure shortwave near-infrared radiances to advance our understanding of processes relevant to shortwave absorption by the climate system, radiative feedbacks, and Earth’s albedo variability with added insight into hemispheric albedo symmetry. We use Nimbus-7 observations, global model simulations and radiative transfer calculations to demonstrate applications of the added spectral knowledge in climate science. Although Libera’s absolute accuracy is unprecedented, it is insufficient to adequately close Earth’s energy budget. We will therefore discuss current and future avenues to indirectly and directly measure EEI from space. The latter is potentially feasible through sensing radiation pressure-induced accelerations acting on near-spherical spacecrafts, which under optimal conditions, are directly proportional to the net radiative flux experienced at the satellite’s location. This approach has been considered in the past, and the mission requirements to achieve a measurement accuracy within 0.3 Wm-2 are currently under investigation.