Results 171 to 180 of about 1,156 (218)

Recruitment of BAG2 to DNAJ-PKAc scaffolds promotes cell survival and resistance to drug-induced apoptosis in fibrolamellar carcinoma. [PDF]

Cell Rep
Lauer SM, Omar MH, Golkowski MG, Kenerson HL, Lee KS, Pascual BC, Lim HC, Forbush K, Smith FD, Gordan JD, Ong SE, Yeung RS, Scott JD.   +12 more
europepmc   +1 more source

Working out measurement overlap in the assessment of maladaptive exercise. [PDF]

Int J Eat Disord
Lampe EW, Schaumberg K, Kolar D, Coniglio K, Cooper M, Chapa DAN, Gorrell S.   +6 more
europepmc   +1 more source

Exploring the Cell Biological and Functional Effects of the First Disease Associated KCC1 Genetic Variant. [PDF]

J Cell Physiol
Bloothooft M, Huang J, Hamze M, Houtman MJC, de Boer TP, van Hasselt PM, Ecker GF, Porcher C, Medina I, van der Heyden MAG.   +9 more
europepmc   +1 more source

Observation of the February 2011 Forbush decrease by the EEE telescopes [PDF]

European Physical Journal Plus, 2011
The Forbush decrease following the large X2 solar flare on mid-February 2011 has been observed by the muon telescopes of the EEE Project, which are located in several Italian sites and at CERN.
M Abbrescia, S Aiola, R Antolini
exaly   +5 more sources

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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

Anisotropic Forbush decrease of 24 March 2024: First look

Advances in Space Research
A strong Forbush decrease, i.e., suppression of the flux of galactic cosmic rays recorded on Earth, was observed by the global network of ground-based neutron monitors (NMs) on 24 – 25 March 2024.
James H Adams
exaly   +2 more sources

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
openaire   +1 more source

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
openaire   +1 more source

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
openaire   +1 more source