Home ]

The Appearance of Sunspot 981 Marked the Beginning of Solar Cycle 24.....ssn# 981 appeared on 04 Jan 2008

Search the Web Site  

The Webmaster is only able to use one hand to type.  Because of that, a dictation program is frequently used.  The program continually scans the dictation and often makes random changes in the text after final (pre-publication) proofreading has been made.

 

Table of Contents
About Search Engine
ACE Satellite
ACTS Satellite
ALERTS, ADVIS
Amateur Radio
Antennas In Space
Archived Pages
ARISS
Asia
Astroid Watch and Information
Atomic Clocks
Aurora Activity
Australia Propagation Report
Auto Updates Solar Conditions
Background Amateur Radio in Space
Band Plan For Digital Modes
Beacon List - International
Beacon Schedule
Black Holes
Bolide Over New Mexico
Broad Band_Power Lines
Bz
CAPS
Cassini Mission
Chandra
Comets
Comet Watch
Comet Watch 2
Communications in Space
Conditions Solar Geomagnetic
Contest
Coordinates of Countries
Coordinates_U.S.
U.S. Land Mark Coordinate Locator
Cosmic Dust
Cosmic Rays
Critical Frequency
Current Conditions List
Daily Photo
Decibel
Deep Space Network
Deep Impact 1
Digital Communications
Disasters Viewed From Space
Download
E10.7 Index
Earthquakes
Eclipse
Eclipse2
ESA News Release
Europe
Explore The Ionosphere In Real-Time
A Final Look at Field Day 2008
Finding the Position of Satellites
Forecast
Genesis Pictures
Genesis_updates
Genesis Special Update Page
Genesis Time Line
Genesis Special Update 2
Geomagnetic Conditions and Forecast
Geomagnetic Data Sources
Geomagnatism
GPS_Problems
Hazardous Space Objects
HF Beacons Region 2
Hurricane Net Frequencies
Ionosonde at San Miguel
Intermagnet
Int. Space Station
Int_Space_Station2
Ionospheric Sounding
ISES Codes
ISS Daily Life
ISS Daily Life 2
Kazakhstan
Kp Index
Links to Important Websites
Links
MARS_Historical_Projects
Medicine
Meteor Scatter
Meteor Shower and Watch
Top Page 1
Missions of Interest
The Deep Impact Mission
Name Change
National Geophysical Data Center
News
NEWS_FCC
New NASA Links
NASA TV
NOAA RSGA Forecast
NOAA_Scales
Orbital Element News
Orbital Element Explanation
Ozone Effects of NOx on Ozone Layers
Perseids Meteor Sho
Propagation_Global
Propagation Gray Line
Propagation_Other Influences
Propagation Programs1
Propagation Programs 2
Proton Event
Radio, A, K-Indices
Radio Detection
Radio Emission
Radio_Meteors
Radio Plasma Imager
Radio Wave Frequency Spectrum
Return To Flight
RSGA Report
Satellite Data Base 1
Satellite Instrumentation
SOHO Condition
Solar Auto Updates
Solar Events Code
Solar Facts and Links
Solar Flares - Recent
Solar Storm Effects on Radio
Solar_Wind
Declining Pressure of the Solar Wind
Solar_wind2
Space Environment Center
Space Flight 1
Space Shuttle Facts
Space Shuttle Facts 2
Space Shuttle Return to Flight
Space Shuttle Tiles 1
Shuttle Tiles 2
Shuttle Tiles Page 3
Space Shuttle Press Release 1
Solar Cycle 24 a new beginning
Space Weather Agencies
Spirit of Knoxville
Stardust Events
Sunspot Counting Methods
Sunspot Number RI
SuperFlare
Synopsis of X-28 Flare
Synoptic Codes for Geophysical Data
T - Index
Time Zone Map
Understanding WWV
UTC Conversion Tables
Values for Solar Activity
World Data Center
WWV
Glossary Page 1.htm
Code of the Ham Radio Operator
Search my web
Propagation Programs
Introduction to Propagation Models
Privacy
Atomic Clock barB

 

IONOSPHERIC SOUNDING 

Ionospheric Profiling

A quick look at an area in transit.

For a number of years we have used the term "Ionospheric Profiling" on the Web Site to describe some of the information collected by Ionosondes.  In the strictest sense, ionospheric profiling includes more information than is usually scaled from the graphical product of a ionosonde - the ionogram. The current method of scaling an ionogram is based on a convention dating from 1989.  Changes are currently being considered.

Ionosondes  sound  the ionosphere using a technique of pulsed radar radiated in a vertical orientation with regards to the Earth's surface. Ionosondes increase the frequency of the radiated signal in a linear fashion with time. The "Time" of signal transmission and the time that the echoed signal is returned to Earth are noted. The difference in time is converted to "Distance" .  Parameters usually scaled from a ionogram include:

  • fmin: The frequency (Mhz*1000) of the lowest return in the ionogram.
  • foE: The frequency (Mhz*10) of the E layer critcal frequency.
  • hE: The virtual height (km) of the E layer.
  • foEs: The highest frequency (Mhz*10) of return from the ordinary component of the sporadic E layer (ES).
  • hEs: The virtual height (km) of the Es layer.
  • foF1: The frequency (Mhz*10) of the F1 layer cusp.
  • hf: The virtual height (km) of the F1 layer.
  • foF2: The top most frequency (Mhz*10) of the ordinary component of F-layer.
  • fxI: The top most frequency (Mhz*10) of the extra-ordinary component of the F-layer.
  • hF2: The virtual height (km) of the F2 layer.

For the purpose of ionospheric sounding we will discuss the scaling of an ionogram here. At a later time additional information on ionospheric profiling will be compiled from its scattered pieces into one place on the Web Site using a single heading.

Ionograms and Critical Frequencies

This list was compiled by the Propagations Studies Committee of the Radio Society of Great Britain.

There will be discrepancies in terms and in the way ionograms are scaled. There is a lack of standardization in ionograms obtained by different ionosondes. (These terms are defined in the Web Site's Glossary)

Critical frequency (fof2) plots for the previous day and 7-day average from . Webmaster's Note: The compiler of this list uses "foF2" to represent "critical frequency". On this Web Site FoF2 signifies the Maximum Usable Frequency (MUF) while F2-Critical Frequency is used to represent the Critical Frequency.

Unfortunately there are discrepancies in the use of these two terms. The discrepancies extend far beyond this specific incidence. Usually the author will describe a term and what that term represents.