... (1965)= 7.50 GV; SF= 256 Times Tabulated Counts Pressure Coefficient=-0.71 %/mb Corrected to 960.0 mb Standard Pressure Comment: 1666 1663 1662 1666 1666 1670 1672 1675 1661 1670 1667 1671 1668 1669 1670 1666 1675 1664 1662 1665 1655 1658 1659 1659 92 02 1 1662 1656 1660 1653 1654 1655 1657 1655 1654 1658 1656 1654 1659 1651 1645 1655 1654 1647 1646 1650 1649 1649 1657 1664 92 02 2 1668 ...

Album : asv-album :: Technical photos :: 2012 ::midzoom1 . ... 800 1655 . 800 1656 . 800 1657 . 800 1658 . 800 1659 . 800 1660 . 800 1661 . 800 1662 . 800 1663 . 800 1664 . 800 1665 . 800 1666 . 800 1667 . 800 1668 . 800 1669 . 800 1670 . 800 1671 . 800 1672 . 800 1673 . 800 1674 . 800 1675 . 800 1676 . 800 1677 . ... Album created by album generator from MarginalHacks by Dave on Mon Jan 19 20:22:30 2015 . ...

Next: Measuring aperture Up: Additional information Previous: Temperature and humidity . Some observatories have accurate information available on atmospheric pressure. If it is routinely available for every measurement, it should go in a column labelled PRESSURE, with the SI unit kPa. Note that pressures read from aneroid (dial-type) barometers are not very accurate, and probably should not be used. Only absolute pressures should be recorded, not values ``corrected to sea level''. ...

... The solar wind pressure variations are associated either with tangential discontinuities or interplanetary shocks , which are intrinsic to the solar wind, or with foreshock pressure pulses generated at the bow shock (Korotova and Sibeck, 1994). ... Korotova, G. I., D. G. Sibeck, Generation of ULF magnetic pulsations in response to sudden variations in solar wind dynamic pressure, in Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves , Geophysical Monograph 81 , 265-271, 1994. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

... It was shown in the early 1980's that spectral lines formed around 1-2.5 x 10 5 K were enhanced in radiance by factors up to 15-25 over the normal quiet Sun. From the dynamical viewpoint, this would suggest a pressure imbalance between the sunspot and the surrounding region. ... Here, the electron density was evaluated over a bright sunspot plume region using lines within the O V 760? multiplet. ... The derived densities in all four regions are indicated. ...