Larval and adult nutrition effects on reproductive traits in the red flour beetle

A Plesnar‐Bielak, KR Woch, MA Małszycki… - Journal of …, 2017 - Wiley Online Library
Variation in individual condition is probably one of the most critical factors affecting the high
levels of diversity in animal fitness components, commonly observed in natural populations. …

[HTML][HTML] Fitness Effects of Thermal Stress Differ Between Outcrossing and Selfing Populations in Caenorhabditis elegans

…, MK Labocha, P Kosztyła, KR Woch… - Evolutionary …, 2017 - Springer
The maintenance of males and outcrossing is widespread, despite considerable costs of
males. By enabling recombination between distinct genotypes, outcrossing may be …

Larval and adult nutrition effects on reproductive traits in the red flour beetle.

AP Bielak, KR Woch, MA Małszycki, ATH Alkhawlany… - 2017 - cabidigitallibrary.org
Variation in individual condition is probably one of the most critical factors affecting the high
levels of diversity in animal fitness components, commonly observed in natural populations. …

Equatorward diffuse auroral emissions at Jupiter: Simultaneous HST and Galileo observations

…, J Gustin, B Bonford, N Krupp, J Woch… - Geophysical …, 2009 - Wiley Online Library
… brightness at the ionospheric counterpart of the boundary (50 kR in the North, 15 kR in
the South) and at the general EDE region (40–100 kR in the North, 10–40 kR in the South). …

Energetic electrons in the inner part of the Jovian magnetosphere and their relation to auroral emissions

AT Tomás, J Woch, N Krupp, A Lagg… - Journal of …, 2004 - Wiley Online Library
… mentioned we found brightness ranges of 32–115 kR and 60–320 kR, respectively. In the
previous work, … The authors found precipitation fluxes of ∼100 kR in the region of 10–25 R J . …

Discontinuity in Jupiter's main auroral oval

…, B Bonfond, N Krupp, J Woch - Journal of …, 2008 - Wiley Online Library
… The brightness derived in this paper considers a conversion factor of count per pixel per
second for 1 kiloRayleigh (kR) of H 2 emission plus Lyman-α different for each filter. In particular…

Polar arcs: New results from Viking UV images

JB Austin, JS Murphree, J Woch - Journal of Geophysical …, 1993 - Wiley Online Library
… A typical value for • is 19 (kR/DN) for 2x2 pixel averaging with an integration time of 1.2 s,
preamp gain of 50 V, and voltage of 807.5 V. The major requirement in order to properly …

Auroral plasma acceleration above Martian magnetic anomalies

…, H Koskinen, E Kallio, J Kozyra, J Woch… - The Mars plasma …, 2007 - Springer
… We also compute the electron energy flux and find that the energy flux is sufficient to
cause weak to medium strong (up to several tens of kR 557.7 nm emissions) aurora at Mars. …

[HTML][HTML] ASPERA-3: Analyser of space plasmas and energetic ions for Mars Express

…, J Kozyra, N Krupp, S Livi, J Woch… - In: Mars Express: the …, 2004 - adsabs.harvard.edu
substantial intrinsic martian magnetic field. Without the magnetic cavity of a magnetosphere
to shield the upper atmosphere from the solar wind, Mars is subject to cometlike atmosphere …

Curvature-driven drift mirror instability in the magnetosphere

J Woch, G Kremser, A Korth, OA Pokhotelov… - Planetary and space …, 1988 - Elsevier
The resonant interaction between low frequency waves and magnetospheric plasma particles
is examined for the case where the field-aligned phase velocity is much less than the …