• Aucun résultat trouvé

[PDF] Top 20 The 2-3 minutes periodicity in the polar aurora and the magnetosphere of Jupiter

Has 10000 "The 2-3 minutes periodicity in the polar aurora and the magnetosphere of Jupiter" found on our website. Below are the top 20 most common "The 2-3 minutes periodicity in the polar aurora and the magnetosphere of Jupiter".

The 2-3 minutes periodicity in the polar aurora and the magnetosphere of Jupiter

The 2-3 minutes periodicity in the polar aurora and the magnetosphere of Jupiter

... Khurana 2 , Aikaterini Radioti 1 , Jacques Gustin 1 INSTITUTIONS (ALL): ...University of Liège, Liège, Belgium. 2. University of California - Los Angeles, Los Angeles, CA, United ...BODY: ... Voir le document complet

2

Spectral observations of transient features in the FUV Jovian polar aurora

Spectral observations of transient features in the FUV Jovian polar aurora

... by the electrons during this event in the 600  12,000 km 2 intercepted by the slit on the ...] The four cases described were selected because they show time variations ... Voir le document complet

11

Six Pieces of Evidence Against the Corotation Enforcement Theory to Explain the Main Aurora at Jupiter

Six Pieces of Evidence Against the Corotation Enforcement Theory to Explain the Main Aurora at Jupiter

... Asymmetry The most direct pieces of evidence of the radially outward flowing currents in the plasma sheet is the azi- muthal bend ‐back of the magnetic ...on ... Voir le document complet

8

The Cassini Campaign observations of the Jupiter aurora by the Ultraviolet Imaging Spectrograph and the Space Telescope Imaging Spectrograph

The Cassini Campaign observations of the Jupiter aurora by the Ultraviolet Imaging Spectrograph and the Space Telescope Imaging Spectrograph

... points of the EUV and FUV on the planet differ by 10,000 ...km. The planet must rotate 8 ◦ ( ∼13 min) to allow the second channel to achieve the same boresight pointing ... Voir le document complet

19

Transient internally driven aurora at Jupiter discovered by Hisaki and the Hubble Space Telescope

Transient internally driven aurora at Jupiter discovered by Hisaki and the Hubble Space Telescope

... by the STIS revealed the brightening of each auroral morphology around the sudden brightening seen in the total auroral power on days 4 and 11 as indicated by the ... Voir le document complet

7

Auroral evidence of Io's control over the magnetosphere of Jupiter

Auroral evidence of Io's control over the magnetosphere of Jupiter

... Motion of the Main Auroral Emissions [ 5 ] The expansion of the main oval on 31 May is not an isolated event, but is part of a continuous increase of the main oval ... Voir le document complet

5

Dynamics of the flares in the active polar region of Jupiter

Dynamics of the flares in the active polar region of Jupiter

... between the moons Io, Europa, and Ganymede produces auroral footprints in the form of localized spots sometimes followed by a tail (see review by Bonfond ...[2012]). The ... Voir le document complet

8

Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions

Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions

... overlapping the H 3 + contribution —has been correlated with the ...H 3 + emission is located. We note that the same spectral signature was not available in the analysis ... Voir le document complet

8

Noncontact atomic force microscopy and density functional theory studies of the (2×2) reconstructions of the polar AlN(0001) surface

Noncontact atomic force microscopy and density functional theory studies of the (2×2) reconstructions of the polar AlN(0001) surface

... During the growth of the AlN(0001) sample at 100 nm/h, the RHEED measurement exhibits a clear (1 × 1) pattern indicating that the surface is not reconstructed or highly ...by the ... Voir le document complet

7

Identification of two new polar tube proteins related to polar tube protein 2 in the microsporidian Antonospora locustae.

Identification of two new polar tube proteins related to polar tube protein 2 in the microsporidian Antonospora locustae.

... present in other insect microsporidia phylogenetically related to ...to the mam- malian microsporidia E. cuniculi and to different insect microsporidian spores, including ...with the extruded ... Voir le document complet

9

Minutes of the Annual General Meeting

Minutes of the Annual General Meeting

... created in partnership between the CHA and Chinook Multimedia. The Millennium Foundation grant is now ...Gaffield and José Igartua for their leadership on this ...that the ... Voir le document complet

2

About periodicity and signal to noise ratio - The strength of the autocorrelation function

About periodicity and signal to noise ratio - The strength of the autocorrelation function

... Abstract In condition monitoring a part of the information necessary for decision-making comes from scrutinizing a time measure or a transform of this ...advantages of the ... Voir le document complet

14

Minutes of the Annual General Meeting

Minutes of the Annual General Meeting

... that the CHA has increased its lobbying ...with the éditorial board of the Globe and Mail and received a sympathetic hearing and a supportive ...éditorial. In ... Voir le document complet

2

Minutes of the Annual General Meeting

Minutes of the Annual General Meeting

... Adoption of minutes from 31 May ...that the CHA Executive and Council decided to use the revenue generated by the spécial sale of CHA booklets to the International ... Voir le document complet

2

X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2

X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2

... 1624-2, the O-type star with the largest known magnetic field (B p ∼ 20 kG), in X-rays with the ACIS-S camera onboard the Chandra X-ray Ob- ...at the minimum and ... Voir le document complet

13

Minutes of the Annual General Meeting

Minutes of the Annual General Meeting

... up in the same letter a number of questions which the CHA executive and Council, as well as the Annual General Meeting, hâve considered sufficiently important to debate ... Voir le document complet

3

Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans

Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans

... examining the absolute magnitude (H) distributions (hereafter HD) of the cold and hot populations in the Kuiper belt and of the Trojans of ... Voir le document complet

24

The L^2 -Alexander torsion of 3-manifolds

The L^2 -Alexander torsion of 3-manifolds

... By the above we have det r N (H) (A) = det N (H) (A), and the desired equality det N (H) (A) = m(det(A)) is proved in [Ra12, Section ...R[S] the R-vector space spanned freely by ... Voir le document complet

47

On a directed variation of the 1-2-3 and 1-2 Conjectures

On a directed variation of the 1-2-3 and 1-2 Conjectures

... Abstract In this paper, we consider the following question, which stands as a directed analogue of the well-known 1-2-3 Conjecture: Given any digraph D with no arc − uv verifying ... Voir le document complet

14

Simultaneous Double Star and Cluster FTEs observations on the dawnside flank of the magnetosphere

Simultaneous Double Star and Cluster FTEs observations on the dawnside flank of the magnetosphere

... Cluster. The detection of high-energy mag- netospheric plasma mixed with low-energy magnetosheath plasma strongly suggests that reconnection was still occur- ring between the magnetosheath and ... Voir le document complet

12

Show all 10000 documents...