Search Publications

A new, lower value of total solar irradiance: Evidence and climate significance
DOI: 10.1029/2010GL045777 Bibcode: 2011GeoRL..38.1706K

Lean, Judith L.; Kopp, Greg

The most accurate value of total solar irradiance during the 2008 solar minimum period is 1360.8 ± 0.5 W m-2 according to measurements from the Total Irradiance Monitor (TIM) on NASA's Solar Radiation and Climate Experiment (SORCE) and a series of new radiometric laboratory tests. This value is significantly lower than the canonical val…

2011 Geophysical Research Letters
SOHO 529
Fermi and betatron acceleration of suprathermal electrons behind dipolarization fronts
DOI: 10.1029/2011GL048528 Bibcode: 2011GeoRL..3816104F

André, M.; Vaivads, A.; Fu, H. S. +1 more

Two dipolarization front (DF) structures observed by Cluster in the Earth midtail region (XGSM ≈ -15 RE), showing respectively the feature of Fermi and betatron acceleration of suprathermal electrons, are studied in detail in this paper. Our results show that Fermi acceleration dominates inside a decaying flux pileup region (…

2011 Geophysical Research Letters
Cluster 337
Strong influence of lunar crustal fields on the solar wind flow
DOI: 10.1029/2010GL046215 Bibcode: 2011GeoRL..38.3202L

Barabash, Stas; Holmström, Mats; Futaana, Yoshifumi +5 more

We discuss the influence of lunar magnetic anomalies on the solar wind and on the lunar surface, based on maps of solar wind proton fluxes deflected by the magnetic anomalies. The maps are produced using data from the Solar WInd Monitor (SWIM) onboard the Chandrayaan-1 spacecraft. We find a high deflection efficiency (average ∼10%, locally ∼50%) o…

2011 Geophysical Research Letters
Chandrayaan-1 123
The composition and structure of the Enceladus plume
DOI: 10.1029/2011GL047415 Bibcode: 2011GeoRL..3811202H

Hansen, C. J.; Hendrix, A. R.; West, R. A. +8 more

The Cassini Ultraviolet Imaging Spectrograph (UVIS) observed an occultation of the Sun by the water vapor plume at the south polar region of Saturn's moon Enceladus. The Extreme Ultraviolet (EUV) spectrum is dominated by the spectral signature of H2O gas, with a nominal line-of-sight column density of 0.90 ± 0.23 × 1016 cm

2011 Geophysical Research Letters
Cassini 115
Dispersion relation analysis of solar wind turbulence
DOI: 10.1029/2010GL046588 Bibcode: 2011GeoRL..38.5101N

Glassmeier, K. -H.; Narita, Y.; Motschmann, U. +2 more

Frequency versus wave number diagram of turbulent magnetic fluctuations in the solar wind was determined for the first time in the wide range over three decades using four Cluster spacecraft. Almost all of the identified waves propagate quasi-perpendicular to the mean magnetic field at various phase speeds, accompanied by a transition from the dom…

2011 Geophysical Research Letters
Cluster 97
The minimal solar activity in 2008-2009 and its implications for long-term climate modeling
DOI: 10.1029/2011GL046658 Bibcode: 2011GeoRL..38.6701S

Schrijver, C. J.; Mewaldt, R. A.; Woods, T. N. +1 more

Variations in the total solar irradiance (TSI) associated with solar activity have been argued to influence the Earth's climate system, in particular when solar activity deviates from the average for a substantial period. One such example is the 17th Century Maunder Minimum during which sunspot numbers were extremely low, as Earth experienced the …

2011 Geophysical Research Letters
SOHO 83
Seasonal changes in Titan's meteorology
DOI: 10.1029/2010GL046266 Bibcode: 2011GeoRL..38.3203T

West, R. A.; Schaller, E. L.; McEwen, A. S. +5 more

The Cassini Imaging Science Subsystem has observed Titan for ∼1/4 Titan year, and we report here the first evidence of seasonal shifts in preferred locations of tropospheric methane clouds. South-polar convective cloud activity, common in late southern summer, has become rare. North-polar and northern mid-latitude clouds appeared during the approa…

2011 Geophysical Research Letters
Cassini 80
A fracture history on Enceladus provides evidence for a global ocean
DOI: 10.1029/2011GL048387 Bibcode: 2011GeoRL..3818201P

Patthoff, D. Alex; Kattenhorn, Simon A.

The region surrounding the south pole of Saturn's moon Enceladus shows a young, pervasively fractured surface that emanates enough heat to be detected by the Cassini spacecraft. To explain the elevated heat and eruptive icy plumes originating from large cracks (informally called “tiger stripes”) in the surface, many models implicitly assume a glob…

2011 Geophysical Research Letters
Cassini 69
Compositional diversity at Theophilus Crater: Understanding the geological context of Mg-spinel bearing central peaks
DOI: 10.1029/2011GL047314 Bibcode: 2011GeoRL..3811201D

Head, J. W.; Dhingra, D.; Pieters, C. M. +3 more

Analysis of high resolution Moon Mineralogy Mapper (M3) data reveals the presence of a prominent Mg-spinel-rich lithology in the central peaks of Theophilus crater on the lunar nearside. Other peak-associated lithologies are comprised of plagioclase, olivine, and pyroxene-bearing materials. A consistent spatial association of Mg-spinel …

2011 Geophysical Research Letters
Chandrayaan-1 61
Average magnetotail electron and proton pitch angle distributions from Cluster PEACE and CIS observations
DOI: 10.1029/2011GL046770 Bibcode: 2011GeoRL..38.6103W

Dandouras, I.; Fazakerley, A. N.; Owen, C. J. +2 more

We present results from the first systematic survey of proton and electron pitch angle distributions in the magnetotail, based on Cluster CIS and PEACE data binned by proton plasma β (βp). The proton distributions conform to the canonical picture of magnetotail ions - a boundary layer made up of Earthward streaming and bidirectional fie…

2011 Geophysical Research Letters
Cluster 59