. ∙ :
. ∙ `_., ┐⌐s%#l
. ∙ `.┌%#S$││$\/*└└²l$$ .
. ∙ `_..,,,.._` . .d││\┘'~` :$$:
. ∙ ` _., ┐⌐s%#S$││$S///S$│││\┐./││/` l$$
` _., ┐⌐s%#S$││$\/*└└²'~`` `└\│$$l' .┌: :$$:
#S$││$\/*└└²'~`` `\' ,│$$$ ┐⌐s%#S$$$l :
l$$ _., ┐⌐s%#S$││S/┐. :$$$││$\/*└└²'~`` .
∙ :$$: .,┐s%#S$││$$$$$$$$$$$$$$$$$: :$$$: . `
:$$. \│$│$$$$$$$$$$$$$$$$$$$$$$$: `\│$/┐._` .
` `$$b `└*/│││$/$$$$$$$$$$$$$$$$: `└\$││$/┐.` .
` `$│\. $$$$$$$$$$$$$│\` :│, `'┘/│$\.
`∙ `\││/┌. l$$$$$$││$\└' .$$$│/┐._ `\││\ `.
` `'┘/│S/┐ . :$$l'~` ,│$$$$$$$$$│S/┐. \$$.
∙ `.┌\$│\└²' l$$: _.┌\│$$$$$$$$$$$$$$$$│b. `l$:
. .d││\┘` :$$l :S│$$$$$$$$$$$$$$$$$$$$$$$$│. :$$:
.` /││/' _.┐s%#S$$: l$$$$$$$$$$$$$$$$$$$$$$$$$$$: :$$:
. /$│/ .┌\│$$$$$$$$$l :$$$$$$$$$$$$$$$$$$$$$$$$$$││ l$l
.$$/ .d│$$$$$$$$$$$$$: l$$$$$$$$$$$$$││$\/*└└²'~`` :$$:
` :$l' :$$$$$$$$$$$$$$$$l :││$\/*└└²'~`` _., ┌$$l
:$$: :$$$$$$$$$$$$││$\*┘ _., ┐⌐s%#S$││$\/*└²''
:$$: ││$\/*└└²'~`` _., ┐⌐s%#S$││$\/*└└²'~`` . ∙ :
l$l _., l$││$\/*└└²'~`` . ∙ ` :
$$: Cl! _., ┐⌐s%#S$││$$l :$$ ∙ ` :
$$l _., ┐⌐s%#S$││$\/*└└²'~`` :$$: l$: :
$$$$││$\/*└└²'~`` . ∙ ` . $$l, ┐⌐s%$││ ∙ :
²'~` . ∙ ` │$\*└²²'~`` . :
:` : . ∙ : ` :
: : :
: ∙ ' ∙ :
: e ┌──── P ┌──── S ── ∙ i ∙ ── L ────┐ O ────┐ n :
: ∙ . ∙ :
: :
: :
: V-Planner v2.00 Keygen Only (c) HHS Software :
: :
: :
: rELEASe dATe [....05-18-2002] - pROGRAm tYPe [.......Utility] :
: cRACKEr [.......EPSiLON Team] - pROTECTIOn [...Serial number] :
: sUPPLiEr [......EPSiLON Team] - dISKS nUMBERs [....01*2.88Mo] :
: pACKAGEr [......EPSiLON Team] - oS [................WinAll] :
: tESTEr [........EPSiLON Team] - diSKSEt iNFOs [epsvp200.zip] :
: :
:......... .......................:
: :
. ∙ . : ................. ... . . :.......................
∙ `.: : :
: :
` .......: r ─ E ─ L ─ E ─ A ─ S ─ E i ─ N ─ F ─ O ─ s :
' ∙ ' :
:
. :
:
∙ :
: V-Planner is a program that uses the Varying Permeability :
: Model (VPM) for deco profiles. VPM is a new decompression :
: model that is well suited to today's technical diving. :
: The deco profiles generally start deeper than traditional :
: methods, and the shallow stops are usually shorter. :
: Ascent ceilings are determined based on allowable :
: gradients for bubble formation rather than M-values. :
: These super saturation gradients are determined by :
: tracking sets of VPM nuclei (bubble seeds) of a certain :
: initial critical radius. These are the microscopic :
: physical structures that stabilize free phase gas and that :
: can grow into full fledged bubbles when the super :
: saturation gradient is sufficient to probe the Laplace :
: condition for bubble formation. :
: :
:....................... .........:
: :
.......................: . . ... ................. : . ∙ .
: : :.` ∙
: :
: i ─ N ─ S ─ T ─ A ─ L ─ L i ─ N ─ F ─ O ─ s :....... `
: ' ∙ '
:
: .
:
: ∙
: Generate a valid serial with our Keygen to remove the :
: shareware restrictions. :
: :
:......... .......................:
: :
. ∙ . : ................. ... . . :.......................
∙ `.: : :
: :
` .......: g ─ R ─ E ─ E ─ T ─ i ─ N ─ G ─ s :
' ∙ ' :
:
. AMN - BS - CLS - CORE - DAMN - ECL - MAGiCAL - MJD :
ORiON - MYTH - PARADOX - SCOTCH - SSG - TMG - TNO - uCF :
∙ :
: :
:...Last.Updated.o8/o5/2oo2................................Ascii.By.Cleaner...: