org.spase.parser200
Enum EnumPhenomenonType

java.lang.Object
  java.lang.Enum<EnumPhenomenonType>
      org.spase.parser200.EnumPhenomenonType

All Implemented Interfaces:

java.io.Serializable, java.lang.Comparable<EnumPhenomenonType>

public enum EnumPhenomenonType
extends java.lang.Enum<EnumPhenomenonType>

Java class for enumPhenomenonType.

The following schema fragment specifies the expected content contained within this class.

 <simpleType name="enumPhenomenonType">
   <restriction base="{http://www.w3.org/2001/XMLSchema}string">
     <enumeration value="ActiveRegion"/>
     <enumeration value="Aurora"/>
     <enumeration value="BowShockCrossing"/>
     <enumeration value="CoronalHole"/>
     <enumeration value="CoronalMassEjection"/>
     <enumeration value="EITWave"/>
     <enumeration value="EnergeticSolarParticleEvent"/>
     <enumeration value="ForbushDecrease"/>
     <enumeration value="GeomagneticStorm"/>
     <enumeration value="InterplanetaryShock"/>
     <enumeration value="MagneticCloud"/>
     <enumeration value="MagnetopauseCrossing"/>
     <enumeration value="RadioBurst"/>
     <enumeration value="SolarFlare"/>
     <enumeration value="SolarWindExtreme"/>
     <enumeration value="Substorm"/>
   </restriction>
 </simpleType>
 

Enum Constant Summary

ACTIVE_REGION
A localized, transient volume of the solar atmosphere in which PLAGEs, SUNSPOTS, FACULAe, FLAREs, etc.

AURORA
An atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force.

BOW_SHOCK_CROSSING
A crossing of the boundary between the undisturbed (except for foreshock effects) solar wind and the shocked, decelerated solar wind of the magnetosheath.

CORONAL_HOLE
An extended region of the corona, exceptionally low in density and associated with unipolar photospheric regions.

CORONAL_MASS_EJECTION
A solar event which involves a burst of plasma which is ejected from the Sun into the interplanetary medium.

EIT_WAVE
A wave in the corona of the Sun which produce shock waves on the Sun’s chromosphere (Moreton Waves).

ENERGETIC_SOLAR_PARTICLE_EVENT
An enhancement of interplanetary fluxes of energetic ions accelerated by interplanetary shocks and/or solar flares.

FORBUSH_DECREASE
A rapid decrease in the observed galactic cosmic ray intensity following the passage of an outwardly convecting interplanetary magnetic field disturbance, such as those associated with large CME's, that sweep some galactic cosmic rays away from Earth.

GEOMAGNETIC_STORM
A magnetospheric disturbance typically defined by variations in the horizontal component of the Earth's surface magnetic field.

INTERPLANETARY_SHOCK
A shock propagating generally antisunward through the slower solar wind, often seen in front of CME-associated plasma clouds.

MAGNETIC_CLOUD
A transient event observed in the solar wind characterized as a region of enhanced magnetic field strength, smooth rotation of the magnetic field vector and low proton density and temperature.

MAGNETOPAUSE_CROSSING
A crossing of the interface between the shocked solar wind in the magnetosheath and the magnetic field and plasma in the magnetosphere.

RADIO_BURST
Emissions of the sun in radio wavelengths from centimeters to dekameters, under both quiet and disturbed conditions.

SOLAR_FLARE
An explosive event in the Sun's atmosphere which produces electromagnetic radiation across the electromagnetic spectrum at multiple wavelengths from long-wave radio to the shortest wavelength gamma rays.

SOLAR_WIND_EXTREME
Intervals of unusually large or small values of solar wind attributes such as flow speed and ion density.

SUBSTORM
A process by which plasma in the magnetotail becomes energized at a fast rate.

Method Summary

static EnumPhenomenonType	fromValue(java.lang.String v)
java.lang.String	value()
static EnumPhenomenonType	valueOf(java.lang.String name) Returns the enum constant of this type with the specified name.
static EnumPhenomenonType[]	values() Returns an array containing the constants of this enum type, in the order they're declared.

Methods inherited from class java.lang.Enum

clone, compareTo, equals, getDeclaringClass, hashCode, name, ordinal, toString, valueOf

Methods inherited from class java.lang.Object

finalize, getClass, notify, notifyAll, wait, wait, wait

Enum Constant Detail

ACTIVE_REGION

public static final EnumPhenomenonType ACTIVE_REGION

A localized, transient volume of the solar atmosphere in which PLAGEs, SUNSPOTS, FACULAe, FLAREs, etc. may be observed.

AURORA

public static final EnumPhenomenonType AURORA

An atmospheric phenomenon consisting of bands of light caused by charged solar particles following the earth's magnetic lines of force.

BOW_SHOCK_CROSSING

public static final EnumPhenomenonType BOW_SHOCK_CROSSING

A crossing of the boundary between the undisturbed (except for foreshock effects) solar wind and the shocked, decelerated solar wind of the magnetosheath.

CORONAL_HOLE

public static final EnumPhenomenonType CORONAL_HOLE

An extended region of the corona, exceptionally low in density and associated with unipolar photospheric regions. A coronal hole can be an "open" magnetic field in the corona and (perhaps) inner heliosphere which has a faster than average outflow (wind); A region of lower than "quiet" ion and electron density in the corona; or a region of lower peak electron temperature in the corona than in the "quiet" corona.

CORONAL_MASS_EJECTION

public static final EnumPhenomenonType CORONAL_MASS_EJECTION

A solar event which involves a burst of plasma which is ejected from the Sun into the interplanetary medium.

EIT_WAVE

public static final EnumPhenomenonType EIT_WAVE

A wave in the corona of the Sun which produce shock waves on the Sun’s chromosphere (Moreton Waves). EIT Waves are produced by large solar flare and expand outward at about 1,000 km/s. It usually appears as a slowly moving diffuse arc of brightening in H-alpha, and may travel for several hundred thousand km.

ENERGETIC_SOLAR_PARTICLE_EVENT

public static final EnumPhenomenonType ENERGETIC_SOLAR_PARTICLE_EVENT

An enhancement of interplanetary fluxes of energetic ions accelerated by interplanetary shocks and/or solar flares.

FORBUSH_DECREASE

public static final EnumPhenomenonType FORBUSH_DECREASE

A rapid decrease in the observed galactic cosmic ray intensity following the passage of an outwardly convecting interplanetary magnetic field disturbance, such as those associated with large CME's, that sweep some galactic cosmic rays away from Earth.

GEOMAGNETIC_STORM

public static final EnumPhenomenonType GEOMAGNETIC_STORM

A magnetospheric disturbance typically defined by variations in the horizontal component of the Earth's surface magnetic field. The variation typically starts with a field enhancement associated with a solar wind pressure pulse and continues with a field depression associated with an enhancement of the diamagnetic magnetospheric ring current.

INTERPLANETARY_SHOCK

public static final EnumPhenomenonType INTERPLANETARY_SHOCK

A shock propagating generally antisunward through the slower solar wind, often seen in front of CME-associated plasma clouds.

MAGNETIC_CLOUD

public static final EnumPhenomenonType MAGNETIC_CLOUD

A transient event observed in the solar wind characterized as a region of enhanced magnetic field strength, smooth rotation of the magnetic field vector and low proton density and temperature.

MAGNETOPAUSE_CROSSING

public static final EnumPhenomenonType MAGNETOPAUSE_CROSSING

A crossing of the interface between the shocked solar wind in the magnetosheath and the magnetic field and plasma in the magnetosphere.

RADIO_BURST

public static final EnumPhenomenonType RADIO_BURST

Emissions of the sun in radio wavelengths from centimeters to dekameters, under both quiet and disturbed conditions. Radio Bursts can be "Type I" consisting of many short, narrow-band bursts in the metric range (300 - 50 MHz).; "Type II" consisting of narrow-band emission that begins in the meter range (300 MHz) and sweeps slowly (tens of minutes) toward dekameter wavelengths (10 MHz).; "Type III" consisting of narrow-band bursts that sweep rapidly (seconds) from decimeter to dekameter wavelengths (500 - 0.5 MHz); and "Type IV" consisting of a smooth continuum of broad-band bursts primarily in the meter range (300 - 30 MHz).

SOLAR_FLARE

public static final EnumPhenomenonType SOLAR_FLARE

An explosive event in the Sun's atmosphere which produces electromagnetic radiation across the electromagnetic spectrum at multiple wavelengths from long-wave radio to the shortest wavelength gamma rays.

SOLAR_WIND_EXTREME

public static final EnumPhenomenonType SOLAR_WIND_EXTREME

Intervals of unusually large or small values of solar wind attributes such as flow speed and ion density.

SUBSTORM

public static final EnumPhenomenonType SUBSTORM

A process by which plasma in the magnetotail becomes energized at a fast rate.

Method Detail

values

public static final EnumPhenomenonType[] values()

Returns an array containing the constants of this enum type, in the order they're declared. This method may be used to iterate over the constants as follows:

for(EnumPhenomenonType c : EnumPhenomenonType.values())
        System.out.println(c);

Returns:

an array containing the constants of this enum type, in the order they're declared

valueOf

public static EnumPhenomenonType valueOf(java.lang.String name)

Returns the enum constant of this type with the specified name. The string must match exactly an identifier used to declare an enum constant in this type. (Extraneous whitespace characters are not permitted.)

Parameters:

name - the name of the enum constant to be returned.

Returns:

the enum constant with the specified name

Throws:

java.lang.IllegalArgumentException - if this enum type has no constant with the specified name

value

public java.lang.String value()

fromValue

public static EnumPhenomenonType fromValue(java.lang.String v)