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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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elease will make the loop shrink, <strong>and</strong> therefore<br />

its current will augment in a way inversely proportional<br />

to its size. By the end of the loop life,<br />

the energy output due to this increased electromagnetic<br />

power may supersede that in gravity<br />

waves. In such a case, plasma in the vicinity of<br />

the string loop will be subject to a strong radiation<br />

pressure, <strong>and</strong> thus thin exp<strong>and</strong>ing plasma<br />

shells will be generated. These dense gas shells<br />

would then eventually be the loci for the formation<br />

of galaxies <strong>and</strong> other structures.<br />

While in st<strong>and</strong>ard scenarios cosmic strings<br />

attract surrounding matter via their gravitational<br />

fields, here instead string loops repel shells of<br />

matter via electromagnetic pressure, forming<br />

large-scale structures on the shell boundaries,<br />

<strong>and</strong>voidsintheshellinteriors. Thismodelisimportantly<br />

constrained by present measurements<br />

of distortions in the 3K cosmic microwave background<br />

radiation, notably by the detectors in the<br />

COBE satellite. See conducting string, cosmic<br />

string, Witten conducting string.<br />

Ottawa 10.7 cm flux The solar radio<br />

flux observed at a wavelength of 10.7 cm (or<br />

2800 MHz) by the Ottawa Radio Observatory<br />

at 1700 UT (local noon) has been accepted as<br />

a st<strong>and</strong>ard measurement of solar fluxes. Normally,<br />

the flux is reported in solar flux units<br />

(1 sfu = 1 × 10 −22 webers m −2 Hz −1 ) The<br />

variations of the 10.7 cm flux, of 2800 MHz<br />

flux as it is sometimes called, is closely associated<br />

with enhanced thermal radiation from solar<br />

active regions, <strong>and</strong> thus to the overall level of<br />

solar activity.<br />

outer core In geophysics, the Earth’s outer<br />

core has an inner radius of 1215 km <strong>and</strong> an outer<br />

radius of 3480 km. It is primarily composed of<br />

molten iron with other components dissolved in<br />

it. Convection in the outer core produces the<br />

geodynamo that generates the Earth’s magnetic<br />

field.<br />

outfall A pipeline placed along the seafloor<br />

to disperse wastewater into the sea.<br />

outflow channel Very large dry river channels<br />

seen on Mars. They typically begin in a region<br />

of jumbled terrain (called chaotic terrain)<br />

<strong>and</strong> cross terrain of various ages, often termi-<br />

© 2001 by CRC Press LLC<br />

overwash<br />

nating in the lower-lying northern plains. The<br />

channels have widths between 10 <strong>and</strong> 100 km<br />

<strong>and</strong> are 400 to over 2000 km in length. Features<br />

associated with outflow channels suggest formation<br />

by catastrophic floods, probably caused by<br />

groundwater breaking out of the source region.<br />

Outflow channels are young, typically with formation<br />

ages less than 3 × 10 9 years.<br />

outgoing longwave radiation (OLR) Infrared<br />

radiation emitted by the Earth toward<br />

the space. The OLR displays strong temporal<br />

<strong>and</strong> spatial variations, affected by surface<br />

temperature, moisture, <strong>and</strong> clouds. The maximum<br />

annual-mean OLR occurs over the Saharan<br />

desert where the surface temperature is high<br />

<strong>and</strong> the atmosphere is dry. Satellite-measured<br />

OLR is used to determine the temperature <strong>and</strong><br />

hence the approximate height of clouds. Over<br />

the tropics where heavy precipitation is caused<br />

mostly by deep convection, OLR can be used as<br />

a proxy of convective activity <strong>and</strong> precipitation<br />

rate.<br />

oval equation The partial differential equation<br />

χ(u) ∂2<br />

∂σ2 <br />

(1 +σ 2 <br />

1 +u2<br />

)α+ +λ(u)<br />

α<br />

∂2α = 0<br />

∂u2 for the unknown functions α =α(σ,u),χ =<br />

χ(u) <strong>and</strong> λ = λ(σ). The field equation describing<br />

stationary <strong>and</strong> axially symmetric spacetimes<br />

in general relativity containing only electric<br />

fields. Additionally, the cylindrical radius<br />

function ρ given by<br />

ρ 2 =<br />

<br />

(1 + σ 2 )α −<br />

3<br />

1 + u2<br />

αλχ<br />

α<br />

is required to be a harmonic function in these<br />

solutions.<br />

overtopping A term used to denote the process<br />

of waves pushing water over the top of a<br />

structure such as a breakwater or jetty.<br />

overturning scale See Ozmidov scale.<br />

overwash A term used to describe the flow of<br />

water across a barrier isl<strong>and</strong> <strong>and</strong> into the bay behind.<br />

An overwash fan of deposited sediments<br />

generally results.<br />

347

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