Search Publications

Variability of Titan's induced magnetotail: Cassini magnetometer observations
DOI: 10.1002/2013JA019608 Bibcode: 2014JGRA..119.2024S

Dougherty, Michele K.; Simon, Sven; Neubauer, Fritz M. +1 more

We study the structure and variability of Titan's magnetotail by analyzing Cassini magnetic field observations from all tail crossings between 2005 and 2013. Titan's magnetotail is strongly affected by fluctuations in the ambient magnetospheric field conditions. Therefore, even Titan flybys with nearly identical trajectories may reveal a completel…

2014 Journal of Geophysical Research (Space Physics)
Cassini 8
Forecast of solar proton flux profiles for well-connected events
DOI: 10.1002/2014JA020333 Bibcode: 2014JGRA..119.9383J

Moon, Yong-Jae; Ji, Eun-Young; Park, Jinhye

We have developed a forecast model of solar proton flux profiles (> 10 MeV channel) for well-connected events. Among 136 solar proton events (SPEs) from 1986 to 2006, we select 49 well-connected ones that are all associated with single X-ray flares stronger than M1 class and start to increase within 4 h after their X-ray peak times. These event…

2014 Journal of Geophysical Research (Space Physics)
SOHO 8
A refined classification of SPEs based on the multienergy channel observations
DOI: 10.1002/2014JA020358 Bibcode: 2014JGRA..119.9419K

Cho, K. -S.; Kim, R. -S.; Park, Y. -D. +2 more

We have investigated characteristics of solar proton events (SPEs) and their association with other types of solar eruption using 42 SPEs observed with SOlar and Heliospheric Observatory/Energetic and Relativistic Nuclei and Electron detector from 1997 to 2012. A velocity dispersion analysis was performed to correctly estimate the onset times of p…

2014 Journal of Geophysical Research (Space Physics)
SOHO 7
An unusual long-lived relativistic electron enhancement event excited by sequential CMEs
DOI: 10.1002/2014JA019797 Bibcode: 2014JGRA..119.9038Y

Yang, Xiao C.; Zhu, Guang W.; Zhang, Xiao X. +3 more

An unusual long-lived intense relativistic electron enhancement event from July to August 2004 is examined using data from Fengyun-1, POES, GOES, ACE, the Cluster Mission, and geomagnetic indices. During the initial 6 days of this event, the observed fluxes in the outer zone enhanced continuously, and their maximum increased from 2.1 × 102

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
Rotational/compressional nature of the magnetopause: Application of the BV technique on a magnetopause case study
DOI: 10.1002/2013JA018927 Bibcode: 2014JGRA..119.1898D

Dorville, Nicolas; Belmont, Gérard; Rezeau, Laurence +2 more

The magnetopause boundary implies two main kinds of variations: a density/temperature gradient and a magnetic field rotation. Other variations are associated with these two, concerning in particular the flow velocity, the electric field, and the plasma composition. Compressional and rotational variations are always observed in a close vicinity of …

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
In situ observations of density cavities extending above the auroral acceleration region
DOI: 10.1002/2014JA019799 Bibcode: 2014JGRA..119.5286A

Karlsson, T.; Marklund, G. T.; Alm, L.

The uppermost part of a stable potential structure in the auroral acceleration region was studied using simultaneous observations of Cluster satellites C1 and C3. Both satellites observe a monotonically decreasing electron density as they ascend through the auroral acceleration region. As C1 exits the top of the auroral acceleration region, the el…

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
Comparison of interplanetary CME arrival times and solar wind parameters based on the WSA-ENLIL model with three cone types and observations
DOI: 10.1002/2014JA020339 Bibcode: 2014JGRA..119.7120J

Moon, Y. -J.; Jang, Soojeong; Na, Hyeonock +1 more

We have made a comparison between coronal mass ejection (CME)-associated shock propagations based on the Wang-Sheeley-Arge (WSA)-ENLIL model using three cone types and in situ observations. For this we use 28 full-halo CMEs, whose cone parameters are determined and their corresponding interplanetary shocks were observed at the Earth, from 2001 to …

2014 Journal of Geophysical Research (Space Physics)
SOHO 7
Cluster observations of hot He+ events in the inner magnetosphere
DOI: 10.1002/2013JA019724 Bibcode: 2014JGRA..119.2706Y

Yamauchi, M.; Dandouras, I.; Nilsson, H. +1 more

In the inner magnetosphere inside 65° invariant latitude, Cluster Ion Spectrometry detected hot He+ events of about a few tens to several hundred eV without the same types of hot H+ signature at the same energy. During the 2001-2006 period when the Cluster orbit was almost constant and approximately north-south symmetric at c…

2014 Journal of Geophysical Research (Space Physics)
Cluster 7
Signals of solar cosmic ray flux variations inferred from the noise in raw CCD solar images taken by SOHO/EIT
DOI: 10.1002/2013JA019142 Bibcode: 2014JGRA..119...88O

Chae, Jongchul; Oh, Suyeon; Yi, Yu +1 more

The noise embedded in the raw data in one scientific discipline has sometimes been proven to be a valuable signal for another discipline, and there are examples throughout science history. The solar images taken by the solid state detectors (CCDs) of the Sun monitoring satellites are usually cleaned by removing the traces of cosmic rays on the raw…

2014 Journal of Geophysical Research (Space Physics)
SOHO 7
Technique for measuring and correcting the Taylor microscale
DOI: 10.1002/2013JA019641 Bibcode: 2014JGRA..119.4256C

Dasso, S.; Matthaeus, W. H.; Smith, C. W. +3 more

We discuss and develop methods to estimate and refine measurements of the Taylor microscale from discrete data sets. To study how well a method works, we construct a time series of discrete data with a known power spectrum and Taylor scale, but with various truncations of the resolution that eliminate higher frequencies in a controlled fashion. We…

2014 Journal of Geophysical Research (Space Physics)
Cluster 7