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The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

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FORTE (Fast On-orbit Recording <strong>of</strong> Transient<br />

Events)<br />

A U.S. Air Force satellite, built by the Los Alamos<br />

National Labora<strong>to</strong>ry <strong>to</strong> study natural and artificial radio<br />

emissions from the ionosphere—information needed <strong>to</strong><br />

develop technology for moni<strong>to</strong>ring nuclear test ban<br />

treaties.<br />

Launch<br />

Date: August 29, 1997<br />

Vehicle: Pegasus XL<br />

Site: Vandenberg Air Force Base<br />

Orbit: 799 × 833 km × 70.0°<br />

Forward, Robert L(ull) (1932–)<br />

A science consultant, writer, and futurist specializing in<br />

studies <strong>of</strong> exotic physical phenomena and future space<br />

exploration with an emphasis on advanced space propulsion.<br />

Forward earned a B.S. in physics from the University<br />

<strong>of</strong> Maryland (1954), an M.S. in applied physics from<br />

the University <strong>of</strong> California, Los Angeles (1958), and a<br />

Ph.D. in gravitational physics from the University <strong>of</strong><br />

Maryland (1965). He worked at the Hughes Aircraft<br />

Research Labs (1956–1987) before forming his own company,<br />

Forward Unlimited. <strong>From</strong> 1983 <strong>to</strong> the present, Forward<br />

has had a series <strong>of</strong> contracts from the Department<br />

<strong>of</strong> Defense and NASA <strong>to</strong> explore new energy sources and<br />

propulsion concepts that could produce breakthroughs<br />

in space power and propulsion. In 1994, he formed Tethers<br />

Unlimited with Robert P. Hoyt <strong>to</strong> develop and market<br />

a new multiline space tether.<br />

Fo<strong>to</strong>n<br />

A series <strong>of</strong> recoverable microgravity science satellites<br />

based on Zenit-class Soviet spy spacecraft <strong>of</strong> the type that<br />

also served as Gagarin’s Vos<strong>to</strong>k capsule. <strong>The</strong> Fo<strong>to</strong>n consists<br />

<strong>of</strong> a spherical reentry capsule sandwiched between a<br />

battery pack that separates before reentry and an expendable<br />

service module with a solid-propellant retro-rocket.<br />

<strong>The</strong> <strong>to</strong>tal mass is about 6.5 <strong>to</strong>ns, <strong>of</strong> which 400 kg is science<br />

payload. Fo<strong>to</strong>n satellites remain in an approximately<br />

215 ×380 km ×63°orbit for 12 days, carrying out<br />

experiments such as materials processing, before deorbiting.<br />

<strong>The</strong> first Fo<strong>to</strong>n was launched on April 16, 1985,<br />

and the most recent, Fo<strong>to</strong>n-12, in 1999.<br />

France 1<br />

A French satellite that investigated the properties <strong>of</strong> the<br />

ionized layers <strong>of</strong> Earth’s atmosphere by observing how<br />

frequency bands 141<br />

very-low-frequency (VLF) waves propagate through the<br />

ionosphere.<br />

Launch<br />

Date: December 6, 1965<br />

Vehicle: Scout X-4<br />

Site: Vandenberg Air Force Base<br />

Orbit: 696 × 707 km × 75.9°<br />

Mass on-orbit: 60 kg<br />

France in space<br />

See Asterix, CERISE, CNES, COROT, Louis<br />

Damblanc, Diamant, ELDO, Eole, ESA, Robert<br />

Esnault-Pelterie, Achille Eyraud, France 1, Jean Froissart,<br />

<strong>From</strong> the Earth <strong>to</strong> the Moon, Hammaguira, Helios<br />

(reconnaissance satellites), Hermes, Jason, Y. P. G. Le<br />

Prieur, NetLander, ONERA, ramjet, Rosetta, SPOT,<br />

Stella, STENTOR, TOPEX/Poseidon, and Tournesol.<br />

free fall<br />

<strong>The</strong> motion <strong>of</strong> an object under the sole influence <strong>of</strong> gravity<br />

and, possibly, drag.<br />

French space agency<br />

See CNES.<br />

frequency<br />

<strong>The</strong> number <strong>of</strong> back-and-forth cycles per second in a<br />

wave or wavelike process. Frequency is measured in hertz<br />

(Hz), after the scientist who first produced and observed<br />

radio waves in the labora<strong>to</strong>ry, and is <strong>of</strong>ten denoted by the<br />

Greek letter ν (nu).<br />

frequency bands<br />

Because the complete radio spectrum is so broad, it is<br />

considered <strong>to</strong> be divided in<strong>to</strong> bands ranging from<br />

extremely low frequency (longest wavelengths) <strong>to</strong><br />

extremely high frequency (shortest wavelengths). (See<br />

table, “General Radio Band Designations.”)<br />

Only a small part <strong>of</strong> this spectrum, from about 1 GHz<br />

<strong>to</strong> a few tens <strong>of</strong> gigahertz, is used for practical radio communications.<br />

International agreements control the usage<br />

and allocation <strong>of</strong> frequencies within this important region.<br />

Communications bands are designated by letters that<br />

appear <strong>to</strong> have been chosen at random—S, C, X, and so on.<br />

Indeed, this is exactly how they were chosen. <strong>The</strong> band letters<br />

were originated in World War II, when references <strong>to</strong><br />

frequency bands needed <strong>to</strong> be kept secret. Most commercial<br />

communications use the C (the first <strong>to</strong> be used), Ku,<br />

K, and Ka bands. <strong>The</strong> shorter wavelength bands, such as<br />

Ka, are used in conjunction with small (including hand-

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