Results 131 to 140 of about 508 (177)

Na⁺/K⁺-ATPase: More than an Electrogenic Pump. [PDF]

Int J Mol Sci
Contreras RG, Torres-Carrillo A, Flores-Maldonado C, Shoshani L, Ponce A.   +4 more
europepmc   +1 more source

Effects of Physical Activity on Disordered Eating Behaviours in Individuals With a Psychotic Disorder. [PDF]

Early Interv Psychiatry
Carrier K, Abdel-Baki A, Thériault L, Karelis AD, Lecomte T, Romain AJ.   +5 more
europepmc   +1 more source

Integrating maintaining theories for addiction and binge-eating pathology: A review of affective and reward-based theories. [PDF]

Clin Psychol Rev
Burr EK, Schaefer LM, Dvorak RD, Wonderlich SA.   +3 more
europepmc   +1 more source

Optimizing renal transporter immunodetection: consequences of freeze-thaw during sample preparation.

Am J Physiol Renal Physiol
Hartman-Houstman HL, Ralph DL, Nelson JW, Palmer LG, Faulkner JE, Sullivan JC, Moronge DM, McDonough AA.   +7 more
europepmc   +1 more source

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Efficiency of Mechanisms for the Formation of Sporadic Forbush Decreases

Bulletin of the Russian Academy of Sciences: Physics, 2023
From the measurements of the neutron monitors world network in the period 1996–2018, 31 strong Forbush decreases (5%) were identified that satisfy the accepted event selection criterion. The superposed epoch analyses is used to determine the consistent spatial distributions of the solar wind parameters and the decrease in cosmic ray density.
A. S. Petukhova, I. S. Petukhov, S. I. Petukhov   +2 more
openaire   +1 more source

Corotating Forbush Decreases

Publications of the Astronomical Society of Australia, 1968
A natural introduction to this topic is a brief discussion of two phenomena observable in interplanetary space near Earth—the energetic storm particle event (ESPE), and the recurrent Forbush decrease.
K. G. McCracken, I. Palmer
openaire   +1 more source

Forbush decreases and $

2019
Non-recurrent short term variations of the galactic cosmic-ray (GCR) flux above 70 MeV n$^{-1}$ were observed between 2016 February 18 and 2017 July 3 aboard the European Space Agency LISA Pathfinder (LPF) mission orbiting around the Lagrange point L1 at 1.5$\times$10$^6$ km from Earth.
Grimani, C., Armano, M., Audley, H., Baird, J., Benella, S., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Fabi, M., Ferraioli, L., Ferroni, V., Finetti, N., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Kudela, K., Laurenza, M., Lobo, J. A., Lloro, I., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Meshksar, N., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T., Telloni, D., Texier, D., Thorpe, J. I., Vetrugno, D., Villani, M., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W. J., Wissel, L., Wittchen, A., Zweifel, P.   +84 more
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Diurnal variation and Forbush decrease

Il Nuovo Cimento, 1961
In this work we discuss the depressions often preceding the most important Forbush decreases by less than 24 h, and certain features of a Forbush decrease such as the rarity of onsets during morning hours, the greater amplitude when they happen during the evening as well as the small increases that sometimes happen during the main decrease.
D. Cattani, M. Galli, P. Randi
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Rigidity Dependence of Forbush Decreases

Publications of the Astronomical Society of Australia, 1992
AbstractIna recent paper, Lockwood et al. (1991) have used IMP spacecraft and Neutron Monitor data to consider the rigidity dependence of three large Forbush Decreases over the energy range 50 MeV to 30 GeV. Some of their conclusions are extrapolated to higher energies.
M. L. Duldig, J. E. Humble
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Asymmetries in the Forbush decreases of the cosmic radiation: 2. Superimposed intensity variations during a Forbush decrease

Journal of Geophysical Research, 1963
Intensity increases or decreases, which are sometimes a strong function of longitude, are frequently found superimposed on the normal behavior of the cosmic-ray intensity during Forbush decreases. A study has been made of these effects utilizing the neutron monitor data from many stations distributed in latitude and longitude. The anisotropies recorded
J. A. Lockwood, H. Razdan
openaire   +1 more source