add FlowDocumentReader Style
This commit is contained in:
NaBian committed
1 parent
28639a263d
commit
955894e265
21 files changed
+355
-197
No files matched your search
@@ -4,197 +4,109 @@
|
||||
xmlns:hc="https://handyorg.github.io/handycontrol"
|
||||
xmlns:langs="clr-namespace:HandyControlDemo.Properties.Langs"
|
||||
Background="{DynamicResource RegionBrush}">
|
||||
<UserControl.Resources>
|
||||
<FlowDocument x:Key="FlowDocumentDemo" x:Shared="False" ColumnWidth="400" IsOptimalParagraphEnabled="True" IsHyphenationEnabled="True">
|
||||
<Section FontSize="12">
|
||||
<Paragraph>
|
||||
<Bold>Neptune</Bold> (planet), major planet in the solar system, eighth planet
|
||||
from the Sun and fourth largest in diameter. Neptune maintains an almost constant
|
||||
distance, about 4,490 million km (about 2,790 million mi), from the Sun. Neptune
|
||||
revolves outside the orbit of Uranus and for most of its orbit moves inside the
|
||||
elliptical path of the outermost planet Pluto (see Solar System). Every 248 years,
|
||||
Pluto’s elliptical orbit brings the planet inside Neptune’s nearly circular orbit
|
||||
for about 20 years, temporarily making Neptune the farthest planet from the Sun.
|
||||
The last time Pluto’s orbit brought it inside Neptune’s orbit was in 1979. In
|
||||
1999 Pluto’s orbit carried it back outside Neptune’s orbit.
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" HorizontalAnchor="PageLeft" HorizontalOffset="100" VerticalOffset="20">
|
||||
<Paragraph FontStyle="Italic" TextAlignment="Left" Background="Beige" Foreground="DarkGreen">
|
||||
Neptune has 72 times Earth's volume...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
<Floater Background="GhostWhite" Width="285" HorizontalAlignment="Left">
|
||||
<Table CellSpacing="5">
|
||||
<Table.Columns>
|
||||
<TableColumn Width="155"/>
|
||||
<TableColumn Width="130"/>
|
||||
</Table.Columns>
|
||||
<TableRowGroup>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="3">
|
||||
<Paragraph>Neptune Stats</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Distance from Sun</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>4,504,000,000 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow FontSize="12" Background="LightGray">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Diameter</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>49,532 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Approximate Mass</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>1.0247e26 kg</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="4">
|
||||
<Paragraph FontSize="10" FontStyle="Italic">
|
||||
Information from the
|
||||
<Hyperlink NavigateUri="http://encarta.msn.com/encnet/refpages/artcenter.aspx">Encarta</Hyperlink>
|
||||
web site.
|
||||
</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
</TableRowGroup>
|
||||
</Table>
|
||||
</Floater>
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
Astronomers believe Neptune has an inner rocky core that is surrounded by a vast
|
||||
ocean of water mixed with rocky material. From the inner core, this ocean extends
|
||||
upward until it meets a gaseous atmosphere of hydrogen, helium, and trace amounts
|
||||
of methane. Neptune has four rings and 11 known moons. Even though Neptune's volume
|
||||
is 72 times Earth’s volume, its mass is only 17.15 times Earth’s mass. Because of
|
||||
its size, scientists classify Neptune—along with Jupiter, Saturn, and Uranus—as
|
||||
one of the giant or Jovian planets (so-called because they resemble Jupiter).
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" TextAlignment="Left" HorizontalAnchor="PageCenter" WrapDirection="Both">
|
||||
<Paragraph FontStyle="Italic" Background="Beige" Foreground="DarkGreen" >
|
||||
Neptune has an orbital period of ~20 years...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
Mathematical theories of astronomy led to the discovery of Neptune. To account for
|
||||
wobbles in the orbit of the planet Uranus, British astronomer John Couch Adams and
|
||||
French astronomer Urbain Jean Joseph Leverrier independently calculated the existence
|
||||
and position of a new planet in 1845 and 1846, respectively. They theorized that the
|
||||
gravitational attraction of this planet for Uranus was causing the wobbles in Uranus’s
|
||||
orbit. Using information from Leverrier, German astronomer Johann Gottfried Galle first
|
||||
observed the planet in 1846.
|
||||
</Paragraph>
|
||||
</Section>
|
||||
</FlowDocument>
|
||||
</UserControl.Resources>
|
||||
<hc:TransitioningContentControl>
|
||||
<TabControl Style="{StaticResource TabControlInLine}">
|
||||
<TabItem Header="{x:Static langs:Lang.FlowDocumentScrollViewer}">
|
||||
<FlowDocumentScrollViewer IsToolBarVisible="True" Width="640" Height="400" Margin="32">
|
||||
<FlowDocument ColumnWidth="400" IsOptimalParagraphEnabled="True" IsHyphenationEnabled="True">
|
||||
<Section FontSize="12">
|
||||
<Paragraph>
|
||||
<Bold>Neptune</Bold> (planet), major planet in the solar system, eighth planet
|
||||
from the Sun and fourth largest in diameter. Neptune maintains an almost constant
|
||||
distance, about 4,490 million km (about 2,790 million mi), from the Sun. Neptune
|
||||
revolves outside the orbit of Uranus and for most of its orbit moves inside the
|
||||
elliptical path of the outermost planet Pluto (see Solar System). Every 248 years,
|
||||
Pluto’s elliptical orbit brings the planet inside Neptune’s nearly circular orbit
|
||||
for about 20 years, temporarily making Neptune the farthest planet from the Sun.
|
||||
The last time Pluto’s orbit brought it inside Neptune’s orbit was in 1979. In
|
||||
1999 Pluto’s orbit carried it back outside Neptune’s orbit.
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" HorizontalAnchor="PageLeft" HorizontalOffset="100" VerticalOffset="20">
|
||||
<Paragraph FontStyle="Italic" TextAlignment="Left" Background="Beige" Foreground="DarkGreen">
|
||||
Neptune has 72 times Earth's volume...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
<Floater Background="GhostWhite" Width="285" HorizontalAlignment="Left">
|
||||
<Table CellSpacing="5">
|
||||
<Table.Columns>
|
||||
<TableColumn Width="155"/>
|
||||
<TableColumn Width="130"/>
|
||||
</Table.Columns>
|
||||
<TableRowGroup>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="3">
|
||||
<Paragraph>Neptune Stats</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Distance from Sun</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>4,504,000,000 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow FontSize="12" Background="LightGray">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Diameter</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>49,532 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Approximate Mass</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>1.0247e26 kg</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="4">
|
||||
<Paragraph FontSize="10" FontStyle="Italic">
|
||||
Information from the
|
||||
<Hyperlink NavigateUri="http://encarta.msn.com/encnet/refpages/artcenter.aspx">Encarta</Hyperlink>
|
||||
web site.
|
||||
</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
</TableRowGroup>
|
||||
</Table>
|
||||
</Floater>
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
Astronomers believe Neptune has an inner rocky core that is surrounded by a vast
|
||||
ocean of water mixed with rocky material. From the inner core, this ocean extends
|
||||
upward until it meets a gaseous atmosphere of hydrogen, helium, and trace amounts
|
||||
of methane. Neptune has four rings and 11 known moons. Even though Neptune's volume
|
||||
is 72 times Earth’s volume, its mass is only 17.15 times Earth’s mass. Because of
|
||||
its size, scientists classify Neptune—along with Jupiter, Saturn, and Uranus—as
|
||||
one of the giant or Jovian planets (so-called because they resemble Jupiter).
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" TextAlignment="Left" HorizontalAnchor="PageCenter" WrapDirection="Both">
|
||||
<Paragraph FontStyle="Italic" Background="Beige" Foreground="DarkGreen" >
|
||||
Neptune has an orbital period of ~20 years...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
Mathematical theories of astronomy led to the discovery of Neptune. To account for
|
||||
wobbles in the orbit of the planet Uranus, British astronomer John Couch Adams and
|
||||
French astronomer Urbain Jean Joseph Leverrier independently calculated the existence
|
||||
and position of a new planet in 1845 and 1846, respectively. They theorized that the
|
||||
gravitational attraction of this planet for Uranus was causing the wobbles in Uranus’s
|
||||
orbit. Using information from Leverrier, German astronomer Johann Gottfried Galle first
|
||||
observed the planet in 1846.
|
||||
</Paragraph>
|
||||
</Section>
|
||||
</FlowDocument>
|
||||
</FlowDocumentScrollViewer>
|
||||
<FlowDocumentScrollViewer Document="{StaticResource FlowDocumentDemo}" IsToolBarVisible="True" Width="640" Height="400" Margin="32"/>
|
||||
</TabItem>
|
||||
<TabItem Header="{x:Static langs:Lang.FlowDocumentPageViewer}">
|
||||
<FlowDocumentPageViewer Width="640" Height="400" Margin="32">
|
||||
<FlowDocument ColumnWidth="400" IsOptimalParagraphEnabled="True" IsHyphenationEnabled="True">
|
||||
<Section FontSize="12">
|
||||
<Paragraph>
|
||||
<Bold>Neptune</Bold> (planet), major planet in the solar system, eighth planet
|
||||
from the Sun and fourth largest in diameter. Neptune maintains an almost constant
|
||||
distance, about 4,490 million km (about 2,790 million mi), from the Sun. Neptune
|
||||
revolves outside the orbit of Uranus and for most of its orbit moves inside the
|
||||
elliptical path of the outermost planet Pluto (see Solar System). Every 248 years,
|
||||
Pluto’s elliptical orbit brings the planet inside Neptune’s nearly circular orbit
|
||||
for about 20 years, temporarily making Neptune the farthest planet from the Sun.
|
||||
The last time Pluto’s orbit brought it inside Neptune’s orbit was in 1979. In
|
||||
1999 Pluto’s orbit carried it back outside Neptune’s orbit.
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" HorizontalAnchor="PageLeft" HorizontalOffset="100" VerticalOffset="20">
|
||||
<Paragraph FontStyle="Italic" TextAlignment="Left" Background="Beige" Foreground="DarkGreen">
|
||||
Neptune has 72 times Earth's volume...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
<Floater Background="GhostWhite" Width="285" HorizontalAlignment="Left">
|
||||
<Table CellSpacing="5">
|
||||
<Table.Columns>
|
||||
<TableColumn Width="155"/>
|
||||
<TableColumn Width="130"/>
|
||||
</Table.Columns>
|
||||
<TableRowGroup>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="3">
|
||||
<Paragraph>Neptune Stats</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Distance from Sun</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>4,504,000,000 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow FontSize="12" Background="LightGray">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Mean Diameter</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>49,532 km</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow Background="LightGoldenrodYellow" FontSize="12">
|
||||
<TableCell>
|
||||
<Paragraph FontWeight="Bold">Approximate Mass</Paragraph>
|
||||
</TableCell>
|
||||
<TableCell>
|
||||
<Paragraph>1.0247e26 kg</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
<TableRow>
|
||||
<TableCell ColumnSpan="4">
|
||||
<Paragraph FontSize="10" FontStyle="Italic">
|
||||
Information from the
|
||||
<Hyperlink NavigateUri="http://encarta.msn.com/encnet/refpages/artcenter.aspx">Encarta</Hyperlink>
|
||||
web site.
|
||||
</Paragraph>
|
||||
</TableCell>
|
||||
</TableRow>
|
||||
</TableRowGroup>
|
||||
</Table>
|
||||
</Floater>
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
Astronomers believe Neptune has an inner rocky core that is surrounded by a vast
|
||||
ocean of water mixed with rocky material. From the inner core, this ocean extends
|
||||
upward until it meets a gaseous atmosphere of hydrogen, helium, and trace amounts
|
||||
of methane. Neptune has four rings and 11 known moons. Even though Neptune's volume
|
||||
is 72 times Earth’s volume, its mass is only 17.15 times Earth’s mass. Because of
|
||||
its size, scientists classify Neptune—along with Jupiter, Saturn, and Uranus—as
|
||||
one of the giant or Jovian planets (so-called because they resemble Jupiter).
|
||||
</Paragraph>
|
||||
<Paragraph>
|
||||
<Figure Width="140" Height="50" Background="GhostWhite" TextAlignment="Left" HorizontalAnchor="PageCenter" WrapDirection="Both">
|
||||
<Paragraph FontStyle="Italic" Background="Beige" Foreground="DarkGreen" >
|
||||
Neptune has an orbital period of ~20 years...
|
||||
</Paragraph>
|
||||
</Figure>
|
||||
Mathematical theories of astronomy led to the discovery of Neptune. To account for
|
||||
wobbles in the orbit of the planet Uranus, British astronomer John Couch Adams and
|
||||
French astronomer Urbain Jean Joseph Leverrier independently calculated the existence
|
||||
and position of a new planet in 1845 and 1846, respectively. They theorized that the
|
||||
gravitational attraction of this planet for Uranus was causing the wobbles in Uranus’s
|
||||
orbit. Using information from Leverrier, German astronomer Johann Gottfried Galle first
|
||||
observed the planet in 1846.
|
||||
</Paragraph>
|
||||
</Section>
|
||||
</FlowDocument>
|
||||
</FlowDocumentPageViewer>
|
||||
<FlowDocumentPageViewer Document="{StaticResource FlowDocumentDemo}" Width="640" Height="400" Margin="32"/>
|
||||
</TabItem>
|
||||
<TabItem Header="{x:Static langs:Lang.FlowDocumentReader}">
|
||||
<FlowDocumentReader Document="{StaticResource FlowDocumentDemo}" Width="640" Height="400" Margin="32"/>
|
||||
</TabItem>
|
||||
</TabControl>
|
||||
</hc:TransitioningContentControl>
|
||||
|
||||
Reference in new issue
Block a user