[PDF] Top 20 The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations
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The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations
... made at large heliocentric distances back towards the ...streams of solar wind with different velocities flow out from the Sun, they interact, with faster flow carried under ... See full document
19
Tidal signatures of the thermospheric mass density and zonal wind at midlatitude: CHAMP and GRACE observations
... Hemisphere, the MSNA (also named Weddell Sea anomaly – WSA) was first observed by ground-based ionosondes in the 1950s ...Bellchambers and Piggott, 1958; Penndorf, 1965) and further ... See full document
12
Plasma waves above the ion cyclotron frequency in the solar wind: a review on observations
... ionized and almost collisionless plasma. A first predictive, theoretical model of solar wind was given by Parker (1958) from an hydrodynamic approach (steady state expansion of a ... See full document
11
SMEI direct, 3-D-reconstruction sky maps, and volumetric analyses, and their comparison with SOHO and STEREO observations
... to the SMEI-observed time-varying signal, the reconstruction includes an unchanging background compo- ...to in-situ measurements near Earth. An average in-situ measurement ... See full document
8
Solar cycle variations of the energetic H/He intensity ratio at high heliolatitudes and in the ecliptic plane
... During the second out-of-ecliptic excursion of Ulysses (1999–2002), the more frequent occurrence of solar energetic particle events resulted in almost continuously high ... See full document
15
How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation
... Abstract. Observations from the second Ulysses fast lati- tude scan show that the global structure of solar wind near solar maximum is much more complex than ... See full document
5
Comparison of wind measurements in the troposphere and mesosphere by VHF/MF radars and in-situ techniques
... vatory in Northern Norway. The results illustrate that wind directions are well estimated by the different methods of ob- ...On the other hand, the radar wind ... See full document
13
Velocity fluctuations in polar solar wind: a comparison between different solar cycles
... Abstract. The polar solar wind is a fast, tenuous and steady flow that, with the exception of a relatively short phase around the Sun’s activity maximum, fills ... See full document
7
Predictions of the arrival time of Coronal Mass Ejections at 1AU: an analysis of the causes of errors
... on the properties of CMEs comes from in situ magnetic field and plasma measurements in the inter- planetary medium (especially at 1 AU), where they are usu- ally ... See full document
11
First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground
... by at- tributing the wave generation process to populations of back- streaming ions at the bow shock which are most likely to occur during times of low cone ...waves in ... See full document
15
Blob formation and acceleration in the solar wind: role of converging flows and viscosity
... state, at least before the completion of the ...investigation of this boundary effect might be of interest from the general perspective of reconnection physics, it ... See full document
12
Study of applying a hybrid standalone wind-photovoltaic generation system
... done in two steps. In the first step, three case studies are ...consists of PV panels, converter, batteries and wind ...only the rated power of wind turbine ... See full document
11
A global study of hot flow anomalies using Cluster multi-spacecraft measurements
... description of the method see Facsk´o et ...that the minimum variance method can mostly be used at low magnetic field ...difficult and almost impossi- ble to use in the ... See full document
20
Performance of different methods for reference evapotranspiration estimation in Jaíba, Brazil
... Priestley-Taylor and Tanner-Pelton were classified as “Very good”, and can still be ...On the other hand, Cunha et al. (2013) found “tolerable” and “intermediate” performance for these methods ... See full document
7
Effects of a solar wind dynamic pressure increase in the magnetosphere and in the ionosphere
... 6a and 6b show snap shots of the magnetic field observations from the 210 MM CPMN, CAN- MOS, CARISMA, GIMA, IMAGE, MACCS, SuperMAG, THEMIS and TGO magnetometer arrays between ... See full document
15
SOCIAL ECONOMY – A FORM OF INCLUSION AND OF ''REACTIVATING'' OF LABOR IN THE CONTEXT OF THE CURRENT CRISIS
... )n the context of the cohesion policy, solidarity must represent a support for development ...self‐help and its success depends a great deal on the capacity and the ... See full document
13
The Impact of E-Commerce Securi ty, and National Environment on Consumer adoption of Intern et Banking in Malaysia and Singapore
... ways of performing the same task (Roger, 1983; Agarwal & Prasad, ...experience and banking need is defined as the degree to which an innovation is viewed as being consistent with ... See full document
20
The spatial relationship between active regions and coronal holes and the occurrence of intense geomagnetic storms throughout the solar activity cycle
... regions and coronal holes should also be a determinant of the geoeectiveness of a solar eruptive ...sizes and positions change through- out the sunspot cycle. During ... See full document
6
Sensitivity of the WRF model to PBL parametrizations and nesting techniques: evaluation of surface wind over complex terrain
... areas of complex terrain like the Alps (Whiteman, ...pers the extrapolation of local observations onto regular grids, which could be used for impact ...bridging the gap between ... See full document
43
A practical field study of performances of solar modules at various positions in Serbia
... The average monthly measured values ofio- cident solar energy on horizontal solar module and calculated values of iocident solar energy on optimally ioclioed and vertical solar module, i[r] ... See full document
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