5th COMPTON Symposium: Diffuse galactic gamma rays

------------------------Sky Maps
1-30 MeV COMPTEL full skymap with sources (waveprogs)
1-30 MeV COMPTEL full skymap without sources (waveprogs)
COMPTEL and EGRET full skymaps
COMPTEL skymos full skymaps 1-3, 3-10 and 10-30 MeV and profiles

------------------------Cosmic rays
explanation of modelling approach
cosmic-ray propagation, interactions, secondaries, gamma rays
galprop model
B/C for reacceration model with v_A=20
10Be reacceleration for reacceleration model
10Be and 26Al with ACE data
isotopic_abundances computed with galprop
B/C and subFe/Fe
36Cl/Cl and 54Mn/Mn
results1

------------------------Gamma rays
gamma spectrum C*
proton spectra*
gamma spectrum HN*
antiprotons MASS91
positrons
electron spectra*
Pohl and Esposito electron fluctuations
electron spectra + Ellison*
synchrotron*
ISRF
gamma spectrum HEMN*
gamma profiles*
Orion emissivity spectrum (Digel)
70-150 MeV latitude profile HEMN*
100-150MeV high-latitude profile (Taormina)
anisotropic scattering sketch*
inner Galaxy spectrum aniso-iso 10526*
hilat spectrum aniso-iso 10526*
hilat spectrum 4526*
hilat spectrum 10526*
gammas/sync for various spectra without reacc
sync for various spectra without reacc
model 4507=E-2.4
gamma spectrum SE
gamma spectrum with source component

Galaxy luminosity spectrum 4 kpc
Galaxy luminosity spectrum 10 kpc
---------------------DIFCOR
DIFCOR intro
DIFCOR IC factors
DIFCOR X
Orion X
DIFCOR gradients
emissivity spectrum
spectrum components 10526
spectrum components 4526
DIFCOR isotropic
DIFCOR isotropic with Stecker
DIFCOR conclusions
Dixon halo
Chen IC

conclusions*
invited conclusions
Texas Conclusions

equation
C, B 3D Galactic distribution

reacceleration
halo height recent values
gradients
gamma spectrum HE

Texas Conclusions

26th ICRC Utah 1999 OG3.2.18 GALPROP developments

intro*
interactions*
galprop model*
equation*
C, B 3D Galactic distribution*
B/C diff-conv no break*
B/C reacc v_A=20 *
10Be reacceleration*
halo height recent values
gradients*
gamma spectrum HEMN*
positrons*
antiprotons*
antiprotons MASS91
results1*
New Developments
overview*
isotopic_abundances*
BC subFe*
10Be 26Al*
36Cl 54Mn*
3He/4He*
conclusions*

synchrotron
gamma spectrum C
proton spectra
gamma spectrum HN
electron spectra
gamma spectrum HE
gamma profiles
latitude profile HEMN

electron spectra + Ellison
proton spectra + Lemoine

B/C diff-conv with break
B/C reacc, various v_A
10Be convection

reacceleration

Taormina 1998 COMPTEL poster Strong et al

layout
title
introduction
why parallel ?
details
background variation
1-30 MeV skymap
1-3 MeV skymap
3-10 MeV skymap
10-30 MeV skymap
1-3 MeV longitude profile
3-10 MeV longitude profile
10-30 MeV longitude profile
1-3 MeV latitude profile
3-10 MeV latitude profile
10-30 MeV latitude profile
spectrum + 4th Compton/Strong
spectrum + OSSE
spectrum + Bloemen etal. (Taormina)
COMPTEL/EGRET skymaps

FINAL PAPER

3rd INTEGRAL Workshop Taormina 1998

Strong & Moskalenko: Diffuse Galactic Continuum models

layout
title
modelling: general
electron spectra
gamma spectrum C
hard electron spectra text......... gamma spectrum HE
EGRET profiles text .......... gamma longitude profile 70-100 MeV ....... gamma longitude profile 4000-10000 MeV
100-150 MeV high latitude profile
synchrotron text.................... synch. spectral index
ISRF
low energy gammas text....... gamma spectrum SE
408MHz longitude,latitude profiles
gamma spectrum HN
gamma spectrum HEMN
antiprotons
positrons

gamma longitude profile 30-50 MeV
gamma longitude profile 50-70 MeV
gamma longitude profile 70-100 MeV
gamma longitude profile 100-150 MeV
gamma longitude profile 150-300 MeV
gamma longitude profile 300-500 MeV
gamma longitude profile 500-1000 MeV
gamma longitude profile 1000-2000 MeV
gamma longitude profile 2000-4000 MeV
gamma longitude profile 4000-10000 MeV

100-150MeV high-latitude profile
gamma polar spectrum
Galaxy luminosity spectrum